| Шығарылым |
Атауы |
Файл |
| Том 100, № 11 (2023) |
NO BIOMARKER: TRANSMISSION AND EMISSION METHODS FOR ITS POTENTIAL DETECTION IN EXOPLANET ATMOSPHERES WITH SPEKTR-UF (WSO-UV) |
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Tsurikov G., Bisikalo D.
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| Том 101, № 9 (2024) |
V839 Cep – a new quadruple doubly eclipsing system |
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Volkov I., Volkova A., Bagaev L.
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| Том 101, № 5 (2024) |
V957 Cep is a Zero-Age Eclipsing System |
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Volkov I., Naroenkov S., Kravtsova A.
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| Том 100, № 5 (2023) |
Adiabatic Radio Emission Spectrum of the Sun’s Coronal Holes |
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Dravskikh A., Dravskikh Y.
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| Том 101, № 2 (2024) |
Adiabatic spectrum of radio emission of plasma clouds, emitted by the Sun during solar flares, and inhomogeneities of the spectrum of radio emission of clouds |
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Dravskikh А., Dravskikh Y.
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| Том 101, № 6 (2024) |
ET Dra activity according to observations in 2018–2023 |
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Savanov I., Naroenkov S., Nalivkin M., Tarasenkov A., Dmitrienko E.
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| Том 100, № 7 (2023) |
THE ACTIVITY OF A SOLAR-TYPE STAR TOI-1422 AND MASS LOSS OF THE ATMOSPHERE OF THE PLANET TOI-1422b |
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Savanov I.
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| Том 100, № 6 (2023) |
Analysis of the Possibilities of Short-Term Prediction of Geomagnetic Perturbations from Observations of Coronal Mass Ejections at the BSA LPI Radio Telescope |
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Lukmanov V., Chashei I., Tyul’bashev S., Subaev I.
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| Том 101, № 8 (2024) |
Analysis of gradient profiles and morphology of the Vela Jr. supernova remnant |
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Pronicheva S., Iyudin A.
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| Том 100, № 3 (2023) |
Analysis of the Parameters of Radio Pulsars with Giant Pulses Using the Principal Component Analysis |
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Malov I., Malov O.
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| Том 101, № 7 (2024) |
Analysis of reasons of the geomagnetic storm on December 1–2, 2023, from interplanetary scintillation observations at the BSA LPI radio telescope |
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Lukmanov V., Chashei I., Tyul’bashev S., Subaev I.
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| Том 100, № 3 (2023) |
GAIA Arguments for and against a Hypothetical Sun Companion |
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Malkov O.
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| Том 100, № 8 (2023) |
ASTRONOMICAL AND COSMOCHEMICAL ASPECTS OF THE LIFE ORIGIN PROBLEM |
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Marov M.
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| Том 100, № 12 (2023) |
AERONOMIC MODEL OF HYDROGEN-HELIUM UPPER ATMOSPHERES OF HOT GIANT EXOPLANETS |
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Zhilkin A., Gladysheva Y., Shematovich V., Bisikalo D.
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| Том 101, № 8 (2024) |
Aeronomy of the atmosphere of ultra-hot Jupiter Kelt9B taking into account the kinetics of hydrogen atom levels |
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Shaikhislamov I., Miroshnichenko I., Rumenskikh M., Shepelin A., Berezutsky A., Sharipov S., Golubovsky M., Chibranov A., Khodachenko M.
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| Том 101, № 6 (2024) |
Force free magnetic flux rope with a high current density on the axis |
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Solov’ev A.
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| Том 101, № 8 (2024) |
Variations in the radiation intensity of the pulsar B0950+08: 9 years of monitoring at a frequency of 110 MHz |
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Smirnova T., Toropov M., Tyul'bashev S.
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| Том 101, № 7 (2024) |
Secular evolution and stability of rings around rotationally asymmetrical bodies. Revisiting the problem |
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Kondratyev B., Kornoukhov V.
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| Том 101, № 9 (2024) |
The [N/C] value as an indicator of the red giant evolution: observed differences between magnetic and non-magnetic giants |
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Lyubimkov L., Poklad D.
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| Том 100, № 7 (2023) |
MILESTONES IN THE DEVELOPMENT OF CELESTIAL MECHANICS |
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Kondratyev B.
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| Том 100, № 11 (2023) |
INTERACTION OF THE EXOPLANET HAT–P–11b WITH THE STELLAR WIND |
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Belenkaya E.
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| Том 101, № 9 (2024) |
The effect of star flare activity on the structure of the hydrogen-helium upper atmosphere of hot Jupiter |
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Zhilkin A., Gladysheva Y., Shematovich V., Tsurikov G., Bisikalo D.
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| Том 100, № 5 (2023) |
Effect of Dust Evaporation and Thermal Instability on Temperature Distribution in a Protoplanetary Disk |
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Pavlyuchenkov Y., Akimkin V., Topchieva A., Vorobyov E.
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| Том 101, № 12 (2024) |
Influence of departures from LTE on determinations of the sulphur abundances in A–K type stars |
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Korotin S., Kiselev K.
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| Том 100, № 1 (2023) |
Influence of Poloidal Magnetic Field on the Parameters and Dynamics of a Plasma Flow Generated in a Plasma-Focus Discharge in a Laboratory Simulation of Jets from Young Stellar Objects |
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Krauz V., Vinogradov V., Kharrasov A., Myalton V., Mitrofanov K., Beskin V., Vinogradova Y., Il’ichev I.
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| Том 101, № 11 (2024) |
The effect of the star high energy radiation flux on the structure of the hydrogen-helium upper atmosphere of hot Jupiter |
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Zhilkin A., Gladysheva Y., Shematovich V., Tsurikov G., Bisikalo D.
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| Том 100, № 10 (2023) |
INFLUENCE OF RADIATION FORCES ON THE OBSERVED POSITION AND EVOLUTION OF THE ORBIT OF SPACE DEBRIS OBJECTS WITH A HIGH AREA-TO-MASS RATIO |
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Sannikova T.
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| Том 100, № 2 (2023) |
Effect of the Eccentricity of the Planet’s Orbit on the Limb Darkening Coefficients of the Eclipsed Star |
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Bekesov E., Cherepashchuk A.
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| Том 100, № 1 (2023) |
Possibilities of the Phase-Contrast X-Ray Method in a Laboratory Astrophysical Experiment on the Study of Plasma Instabilities |
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Makarov S., Pikuz S.
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| Том 100, № 11 (2023) |
ON THE POSSIBILITY OF ESTIMATION OF THE ORBIT ECCENTRICITY OF A BINARY SYSTEM WITH AN EXOPLANET USING A TRANSIT LIGHT CURVE |
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Bekesov E., Abubekerov M., Gostev N., Cherepashchuk A.
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| Том 101, № 7 (2024) |
Rotation of the Milky Way halo in the solar neighborhood based on GAIA DR3 catalog |
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Tkachenko R., Bryndina A., Zhmailova A., Korchagin V.
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| Том 101, № 2 (2024) |
Rotation of the apsidal line in the eclipsing system V1059 Cep |
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Kozyreva V., Khamrakulov F., Burkhonov O., Bogomazov A., Satovskiy B.
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| Том 101, № 6 (2024) |
Time structure of the average rotation measure for accretion disk in shearing box approximation |
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Buldakov M., Andrianov A.
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| Том 101, № 11 (2024) |
Flare June 7, 2011, and analysis of eruptive prominence fragments |
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Kupryakov Y., Bychkov K., Maliutin V., Gorshkov A., Belova O.
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| Том 100, № 12 (2023) |
LUMINOSITY OUTBURSTS IN INTERACTING PROTOPLANETARY SYSTEMS |
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Skliarevskii A., Vorobyov E.
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| Том 101, № 5 (2024) |
Gas-Dynamical Model of Accretion on a Neutron Star with Viscosity and the Influence of Large-Scale Vortices on the Transmission of Angular Momentum |
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Aksenov A., Chechetkin V.
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| Том 100, № 12 (2023) |
DARK MATTER HALOS IN NUMERICAL MODELS AT REDSHIFTS 0 ≤ z ≤ 9 |
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Demyanskii M., Doroshkevich A., Larchenkova T., Pilipenko S.
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| Том 101, № 3 (2024) |
Global families of periodic orbits adjacent to libration points in the restricted three-body problem |
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Tkhai V.
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| Том 100, № 11 (2023) |
NEXT GENERATION GRAVITY MISSIONS: STUDYING THE POSSIBILITIES OF MULTIPLE CONSTELLATION |
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Filetkin A., Zhamkov A., Ayukov S., Milyukov V.
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| Том 100, № 11 (2023) |
GRAVITATIONAL CAPTURE AS A POSSIBLE SCENARIO ORIGIN OF THE MOON |
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Tutukov A., Dremova G., Dremov V.
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| Том 101, № 4 (2024) |
Dynamics of the plasma ejection structure in laboratory modeling of young star jets at plasma focus facilities |
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Kalashnikov I., Beskin V., Krauz V.
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| Том 101, № 4 (2024) |
Dynamic processes in current sheets and experimental laboratory astrophysics |
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Frank А., Kyrie N., Savinov S., Nugaev I., Kharlachev D., Ivanov V., Stepakhin V.
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| Том 100, № 5 (2023) |
Dynamic Study of the Triple Star T Tauri |
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Kiyaeva O., Romanenko L.
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| Том 100, № 5 (2023) |
Dependences of Characteristics of Bulges on the Mass of the Central Black Hole and Theoretical Aspects of Their Origin |
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Botirov F., Nuritdinov S., Ashurov A.
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| Том 100, № 4 (2023) |
Star Structure of the Northern Part of the Orion Sword Region |
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Vereshchagin S., Chupina N.
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| Том 101, № 3 (2024) |
Probing the ionosphere with pulses from the pulsar B2016+28 at a frequency of 324 MHz |
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Burgin M., Popov M.
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| Том 101, № 1 (2024) |
Orbital Period Variations of the Eclipsing Binaries RW Cap, BG Peg, and CU Peg |
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Khaliullina A.
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| Том 100, № 6 (2023) |
Orbital Period Variations of the Eclipsing Binaries RX Ari and V449 Oph |
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Khaliullina A.
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| Том 101, № 11 (2024) |
Variations in the orbital periods of eclipsing binaries δ Lib and SX Lyn |
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Khaliullina A.
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| Том 101, № 11 (2024) |
Measurement of radio emission scattering parameters in the direction of pulsars B0809+74, B0919+06 and B1133+16 with ground-space interferometer RadioAstron |
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Fadeev E., Andrianov A., Burgin M., Popov M., Rudnitskiy A., Smirnova T., Soglasnov V.
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| Том 101, № 1 (2024) |
Image of a black hole illuminated by a parabolic screen |
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Mikheeva E., Repin S., Lukash V.
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| Том 101, № 7 (2024) |
Interpretation of the transit light curve in the presence of one principal minimum taking into account the eccentricity of the transit (planet) orbit |
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Abubekerov M., Gostev N.
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| Том 101, № 2 (2024) |
Study of the rapid variability of a dwarf nova SS Cyg at different brightness levels |
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Khruzina T., Voloshina I., Metlov V.
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| Том 100, № 6 (2023) |
Investigation of the Effect of the Errors of Limb Darkening Coefficients on the Geometric Parameters of a Binary System with an Exoplanet |
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Abubekerov M., Gostev N.
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| Том 101, № 11 (2024) |
Investigation of the temporal variations in scattering and dispersion measure of Giant Radio Pulses in the pulsar в0531+21 in the Crab Nebula at 111 MHz frequency in 2002–2024 |
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Losovsky B., Potapov V.
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| Том 100, № 7 (2023) |
INVESTIGATION OF THE MAGNETIC FIELD FROM OBSERVATIONS OF THE OH MASER IN THE G10.624–0.385 STAR FORMATION REGION |
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Ashimbaeva N., Lekht E., Krasnov V., Tolmachev A.
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| Том 100, № 7 (2023) |
INVESTIGATION OF OH 18 CM MASER EMISSION AND MAGNETIC FIELD IN THE S128 STAR FORMATION REGION |
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Ashimbaeva N., Lekht E., Krasnov V., Tolmachev A.
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| Том 101, № 9 (2024) |
Study of maser emission in 18 cm lines in the star formation region G 109.871+2.114 (Cep A) |
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Lekht E., Ashimbaeva N., Krasnov V., Shoutenkov V.
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| Том 101, № 5 (2024) |
Study of H2O and OH Masers in the Region Formation of a Young High Mass Stellar Object (S255 NIRS 3) |
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Ashimbaeva N., Lekht E., Krasnov V., Shutenkov V.
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| Том 100, № 3 (2023) |
A Study of Variability of the Stokes Parameters and the Magnetic Field of G43.8–0.1 in the OH Line 1665 MHz |
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Ashimbaeva N., Lekht E., Krasnov V., Tolmachev A.
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| Том 100, № 11 (2023) |
TO THE QUESTION OF THE LOCALIZATION OF CME GENERATION ON THE SUN |
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Yazev S., Tomozov V.
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| Том 100, № 3 (2023) |
On the Question of the Primordial Helium Abundance by the RRL Observations in Orion A |
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Tsivilev A., Krasnov V.
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| Том 101, № 12 (2024) |
To the question of north-south asymmetry of solar activity in the 25th Schwabe-Wolf cycle |
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Yazev S., Isaeva Е., Tomozov V., Ivanov K., Hos-Erdene B.
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| Том 100, № 9 (2023) |
CALIBRATING GAIA DR3 UNCERTAINTIES BASED ON DATA FOR WIDE BINARY STARS OF THE FIELD OF GALAXY |
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Kovaleva D.
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| Том 100, № 5 (2023) |
The Exo-Jupiter Candidate FL Lyr b in Data of Kepler and TESS Space Missions |
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Kozyreva V., Bogomazov A., Demkov B., Zotov L., Tutukov A.
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| Том 100, № 6 (2023) |
The Catalog of Resolved Spectroscopic Binaries: Development and Description |
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Zeleke D., Pakhomova P., Tessema S., Negu S., Malkov O.
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| Том 100, № 12 (2023) |
KINEMATICS OF HIGH-SPEED STARS WITHIN 300 PCS FROM THE SUN ACCORDING TO GAIA DR3 |
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Tutukov A., Chupina N., Vereshchagin S.
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| Том 101, № 9 (2024) |
Kinematics of fainst stars of the Sco-Cen association according to Gaia catalog |
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Bobylev V., Bajkova A.
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| Том 100, № 10 (2023) |
KINETIC MODEL OF THE STELLAR WIND FORCING ON THE EXTENDED HYDROGEN ATMOSPHERE OF THE EXOPLANEt π Men c |
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Avtaeva A., Shematovich V.
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| Том 101, № 5 (2024) |
Constructing an Entropy-Force Model of the Expansion of the Universe due to Gravitationally Induced Production of Dark Matter |
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Marov M., Kolesnichenko A.
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| Том 100, № 6 (2023) |
Corotating Disturbances of the Solar Wind in the Monitoring Data of Interplanetary Scintillations: Simulation and Observation |
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Lukmanov V., Chashei I., Tyul’bashev S., Subaev I.
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| Том 100, № 3 (2023) |
Large-Scale Convection during Gravitational Collapse with Neutrino Transport in 2D and 3D Models on Fine Grids |
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Aksenov A., Chechetkin V.
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| Том 101, № 2 (2024) |
Linear polarization of the helium D3 line by accelerated protons in the solar chromosphere |
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Shapochkin M., Bogachev S.
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| Том 100, № 12 (2023) |
RADIATIVE TRANSFER: ASYMPTOTIC SOLUTION OF THE KINETIC EQUATION OF RADIATION PROPAGATION, N-th ORDER ASYMPTOTIC APPROXIMATION AND IMPROVED BOUNDARY CONDITIONS |
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Serov S., Serova S.
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| Том 100, № 9 (2023) |
DEDICATION TO MARIJ ANATOLYEVICH SVECHNIKOV |
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Polushina T.
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| Том 100, № 6 (2023) |
Mass Computations of the Brightness of Stars in an Arbitrary Spectral Band |
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Prokhorov M., Zakharov A., Moshkalev V., Krusanova N., Tuchin M.
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| Том 100, № 11 (2023) |
SCALE-INVARIANT MODE IN COLLISIONLESS SPHERICAL STELLAR SYSTEMS |
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Polyachenko E., Shukhman I.
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| Том 101, № 4 (2024) |
MHD simulations of astrophysical and laboratory jets under different magnetic field configurations |
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Toropina О., Bisnovatyi-Kogan G., Moiseenko S.
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| Том 101, № 1 (2024) |
MHD modeling of the molecular filament evolution |
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Sultanov I., Khaibrakhmanov S.
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| Том 101, № 8 (2024) |
Interstellar scintillation of sources B0821+394 and B1812+412 according to observations on the LPA LPI radio telescope |
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Tyul'bashev S., Chashei I., Grishanova I., Tyul'basheva G., Subaev I.
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| Том 101, № 5 (2024) |
Metallicity and Kinematics of the Circumsolar Stellar Population of the Galaxy |
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Tutukov A., Chupina N., Vereshchagin S.
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| Том 100, № 6 (2023) |
Method of Circular Gaussian Rings in Perturbation Theory |
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Kondratyev B., Kornoukhov V.
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| Том 101, № 4 (2024) |
A method for estimating the number of regolith particles in a dust cloud in a discharge initiated by gyrotron radiation |
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Sokolov A., Gayanova Т., Kozak А., Malakhov D., Nugaev I., Kharlachev D., Stepakhin V.
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| Том 101, № 5 (2024) |
Microstructure in Radio Emission of the Pulsar B1133+16 at a Frequency of 111 MHz |
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Popov M.
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| Том 101, № 6 (2024) |
Long-term optical spectroscopy of B[e] star CI Cam in a quiet state |
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Klochkova V., Miroshnichenko A., Panchuk V.
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| Том 101, № 6 (2024) |
Multi-frequency synthesis in space very long baseline radio interferometry |
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Rudnitskiy A., Shchurov M., Chernov S.
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| Том 100, № 1 (2023) |
Simulation of the “Central Engine” of Astrophysical Jets within the Plasma Focus Facility |
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Beskin V.
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| Том 101, № 4 (2024) |
Model of astrophysical jets in magnetic fields of laser relativistic plasmas |
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Belyaev V., Krainov V., Matafonov А.
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| Том 100, № 12 (2023) |
SIMULATIONS OF LINEAR POLARIZATION OF PRECESSING AGN JETS AT PARSEC SCALES |
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Todorov R., Kravchenko E., Pashchenko I., Pushkarev A.
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| Том 101, № 1 (2024) |
Modeling of the exoplanet HAT-P-11b magnetosphere |
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Belenkaya E., Alexeev I., Kalegaev V.
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| Том 100, № 3 (2023) |
Modeling of Absorption in the Hα Line for the Exoplanet WASP-52b |
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Sharipov S., Miroshnichenko I., Shaikhislamov I.
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| Том 101, № 10 (2024) |
Simulation of the free fall of a gas stream on a protoplanetary disk |
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Grigoryev V., Demidova T.
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| Том 100, № 10 (2023) |
MODIFIED SHAO SPECTROGRAPH FOR SPECTRA WITH LOW RESOLUTION |
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Ismailov N., Alyshov S., Ismailova S., Huseynova F.
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| Том 100, № 10 (2023) |
OBSERVATIONS OF THE FAST RADIO BURST FRB 20220912A ON THE BSA FIAN AND FAST RADIO TELESCOPES |
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Fedorova V., Huang Y., Zhang J., Wang P., Li D., Li X., Dong X., Zhang Z., Rodin A., Xu F.
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| Том 100, № 3 (2023) |
Observations of Hydroxyl in the Onsala 1 Source at 18 cm |
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Ashimbaeva N., Lekht E., Krasnov V., Tolmachev A.
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| Том 100, № 6 (2023) |
Neural Networks for Searching for Meteoral Signals in the Data of the Orbital Telescope “UV Atmosphere” |
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Zotov M., Sokolinskii D., Arifullin A.
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| Том 100, № 8 (2023) |
NEUTRON STARS IN A UNIFORM DENSITY APPROXIMATION |
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Bisnovatyi-Kogan G., Patraman E.
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| Том 101, № 2 (2024) |
Unresolved binary systems with white dwarfs in open star clusters |
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Mikhnevich V., Seleznev A.
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| Том 101, № 8 (2024) |
Non-thermal processes of nitrogen oxide formation during precipitation of auroral electrons into the upper atmospheres of terrestrial planets |
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Shematovich V., Bisikalo D., Tsurikov G., Zhilkin A.
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| Том 101, № 10 (2024) |
New formula for the angular velocity of rotation of liquid equilibrium figures |
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Kondratyev B.
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| Том 100, № 4 (2023) |
New Value of Apsidal Motion Velocity and Physical Parameters of the Triple Eclipsing System AS Cam |
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Volkov I.
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| Том 100, № 8 (2023) |
NEW FORMS OF MATTER IN THE UNIVERSE |
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Cherepashchuk A.
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| Том 101, № 10 (2024) |
New look at the structure of the nearest circumstellar environment of the weak-line T tauri star V718 Per |
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Grinin V., Safonov B., Efimova N., Barsunova O., Strachov I., Borman G., Shugarov S.
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| Том 101, № 3 (2024) |
Displacement norm in the presence of an inverse-square perturbing acceleration in the reference frame associated with the radius vector |
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Sannikova T.
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| Том 101, № 4 (2024) |
On the possibility of studying the effect of magnetic reconnection in a laboratory astrophysical experiment using X-ray emission L-spectra of multiply charged ions |
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Alkhimova М., Makarov S., Skobelev I., Ryazantsev S., Filippov E.
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| Том 100, № 2 (2023) |
On the Possibility of Observing Nitric Oxide on Terrestrial Exoplanets Using the WSO-UV Observatory |
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Tsurikov G., Bisikalo D.
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| Том 100, № 1 (2023) |
Laboratory Simulation of Photosynthesis in a Wide Range of Electromagnetic and Radiation Environment Parameters |
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Grinberg M., Vodeneev V., Il’in N., Mareev E.
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| Том 100, № 2 (2023) |
On the Problems of Detecting Fast Radio Bursts with the LPA LPI |
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Brylyakova E., Tyul’bashev S.
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| Том 100, № 2 (2023) |
On the Evolution of Angles between the Magnetic Moment and the Axis of Rotation in Radio Pulsars |
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Malov I., Malov O.
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| Том 101, № 8 (2024) |
A survey of high mass star forming regions in the line of singly deuterated ammonia NH2D |
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Trofimova E., Zinchenko I., Zemlyanukha P., Thomasson M.
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| Том 100, № 6 (2023) |
Detection of Two New RRATs at 111 MHz |
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Samodurov V., Tyul’bashev S., Toropov M., Dolgushev A., Oreshko V., Logvinenko S.
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| Том 101, № 6 (2024) |
The detection and investigation of exoplanets with MASTER Global network telescopes |
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Lipunov V., Tarasenkov A., Kuznetsov A., Balanutsa P., Antipov G., Kechin Y., Tyurina N., Gorbovskoy E., Buckley D., Francile C., Podesta F., Tlatov A., Rebolo Lopez R., Budnev N., Gress O., Yurkov V.
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| Том 101, № 7 (2024) |
Determination of dynamic and physical characteristics of near-Earth asteroids based on observations from 2022–2023 |
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Kuznetsov Е., Wiebe Y., Glamazda D., Kaiser G., Krushinsky V., Kryuchkov M., Naroenkov S., Perminov A.
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| Том 101, № 5 (2024) |
Determination of Parameters of the Gravity Field of the Earth by Gradiometric Measurements in an Earth-Fixed Reference Frame |
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Klyuykov A.
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| Том 100, № 9 (2023) |
DETERMINATION OF THE CLOSE BINARY SYSTEMS PARAMETERS BY SYNTHESIS METHODS: FROM WHITE DWARFS TO WOLF–RAYET STARS AND BLACK HOLES |
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Antokhina E., Antokhin I.
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| Том 101, № 8 (2024) |
Determining the structure of the atmosphere exoplanet HD 189733 b based on multicolor photometric transit observations |
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Bekesov E.
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| Том 100, № 12 (2023) |
HIGH RESOLUTION OPTICAL SPECTRA OF THE DORMANT LBV STAR P Cyg |
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Klochkova V., Panchuk V., Tavolzhanskaya N.
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| Том 100, № 1 (2023) |
Features of Dynamics and Instability of Plasma Jets Expanding into an External Magnetic Field in Laboratory Experiments with Compact Coaxial Plasma Generators on a Large-Scale “Krot” Stand |
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Korobkov S., Nikolenko A., Gushchin M., Strikovsky A., Zudin I., Aidakina N., Shaikhislamov I., Rumenskikh M., Zemskov R., Starodubtsev M.
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| Том 100, № 9 (2023) |
PECULIARITIES OF LONG-TERM SPOT ACTIVITY OF SOME LATE SPECTRAL-TYPE STARS |
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Kozhevnikova A., Alekseev I., Kozhevnikov V.
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| Том 101, № 7 (2024) |
Peculiarities of radio pulsars with long periods |
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Malov I.
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| Том 101, № 11 (2024) |
Details of modelling the non-stationary thermal structure of an axially symmetric protoplanetary disk |
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Pavlyuchenkov Y.
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| Том 101, № 3 (2024) |
National software for processing information of the satellite – satellite space geodetic system |
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Zhamkov A., Ayukov S., Filetkin A., Milyukov V., Vlasov I., Sementsov V., Gusev I., Zharov V.
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| Том 101, № 8 (2024) |
Fundamental plane distances and peculiar velicities of 140 groups and clusters of galaxies at low redshifts: the Hubble diagram |
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Kopylova F., Kopylov A.
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| Том 101, № 3 (2024) |
Estimation of the spin of a supermassive black hole in Sagittarius A* |
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Andrianov A., Chernov S.
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| Том 101, № 9 (2024) |
Proton fluxes of solar-type stars with planetary systems |
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Savanov I.
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| Том 101, № 2 (2024) |
Pavel Petrovich Parenago and his name in science |
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Kuznetsova I., Prokhorov М.
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| Том 101, № 7 (2024) |
Parameters of star formation regions in galaxies NGC 3963 and NGC 7292 |
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Gusev А., Sakhibov F., Moiseev A., Kostiuk V., Oparin D.
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| Том 100, № 11 (2023) |
PARAMETERS OF RADIO PULSARS AT DIFFERENT DISTANCES FROM THE “DEATH LINE” |
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Ken’ko Z., Malov I.
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| Том 100, № 12 (2023) |
PECULIAR SPECTRUM OF THE WATER MASER IN THE DARK NEBULA MSXDCG24.33+011(G24.33+014) |
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Val’tts I.
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| Том 101, № 3 (2024) |
Transition from super-alfvenic to sub-alfvenic stellar wind flow passing by an exoplanet, using the example of HD 209458b |
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Belenkaya E.
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| Том 100, № 7 (2023) |
PROSPECTS FOR OBSERVING BINARY SUPERMASSIVE BLACK HOLES WITH THE SPACE RADIOINTERFEROMETER |
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Malinovsky A., Mikheeva E.
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| Том 100, № 11 (2023) |
A PLANET OR PRIMORDIAL BLACK HOLE IN THE OUTER REGION OF THE SOLAR SYSTEM AND THE DUST FLOW NEAR EARTH’S ORBIT |
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Eroshenko Y., Popova E.
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| Том 100, № 9 (2023) |
CONFIRMATION OF THE NEW EVOLUTIONARY STATUS OF UU CAS |
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Gorda S.
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| Том 101, № 12 (2024) |
Search for pulsars with periods of more than two seconds at declinations from +21◦ to +42◦ |
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Tyul’bashev S., Tyul’basheva G.
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| Том 101, № 12 (2024) |
Search for interpulses in a complete sample of pulsars at a frequency of 111 MHz |
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Toropov M., Tyul’bashev S., Beskin V.
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| Том 100, № 2 (2023) |
Search for Pulsars in an Area with Coordinates 3h < α < 4h and +21° < δ < +42° |
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Tyul’bashev S., Tyul’basheva G.
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| Том 101, № 12 (2024) |
Search for weak components in pulsar radiation |
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Smirnova T., Toropov M., Tyul’bashev S.
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| Том 100, № 3 (2023) |
Search for Solar Sources of Interplanetary Coronal Mass Ejections Using the Reverse Model of Magnetodynamic Interaction of the Solar Wind in the Heliosphere |
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Rodkin D., Slemzin V., Shugay Y.
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| Том 101, № 2 (2024) |
Polarimetric monitoring of primitive asteroids near perihelion in order to detect their sublimation-dust activity |
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Busarev V., Kiselev N., Shcherbina M., Karpov N., Gorshkov A.
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| Том 101, № 1 (2024) |
Gnevishev-Ohl rule: current status |
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Nagovitsyn Y., Osipova A., Ivanov V.
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| Том 100, № 1 (2023) |
Precision Measurements of X-Ray Spectra for the Diagnosis of Laboratory Astrophysical Plasma |
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Ryazantsev S., Skobelev I., Kuznetsov A., Kulikov R., Pikuz S.
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| Том 101, № 3 (2024) |
Principles of the wave dark matter detection in gravitational redshift experiments in the Solar System |
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Pilipenko S., Litvinov D., Zakhvatkin M., Filetkin A.
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| Том 100, № 8 (2023) |
PROBLEMS OF THE ORIGIN OF THE UNIVERSE |
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Novikov I.
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| Том 101, № 2 (2024) |
Prediction of geomagnetic storms associated with interplanetary coronal mass ejections |
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Rodkin D., Slemzin V.
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| Том 100, № 7 (2023) |
LONG MAGNETIC MINIMUM OF HD 166620 – POSSIBLE BEGINNING OF THE ANALOGUE OF THE MAUNDER MINIMUM |
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Savanov I.
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| Том 101, № 2 (2024) |
Profiles and some dynamic parameters of a layered inhomogeneous elliptical galaxy |
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Gasanov S.
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| Том 100, № 1 (2023) |
Dust Particles in Space: Opportunities for Experimental Research |
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Kuznetsov I., Zakharov A., Zelenyi L., Popel S., Morozova T., Shashkova I., Dolnikov G., Lyash A., Dubov A., Viktorov M., Topchieva A., Klumov B., Usachev A., Lisin E., Vasiliev M., Petrov O., Poroikov A.
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| Том 101, № 10 (2024) |
Starspot activity of the red dwarf star V772 Her |
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Alekseev I., Kozhevnikova A., Kozhevnikov V.
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| Том 101, № 12 (2024) |
Spot and flare activity of single G5 III IV giant HD 199178 from TESS observations |
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Savanov I., Tarasenkov A., Dmitrienko E.
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| Том 101, № 10 (2024) |
Destruction of open star clusters and the radius-mass relationship |
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Tutukov A., Vereshchagin S., Chupina N.
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| Нәтижелер 198 - 1/150 |
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