Detection of Radio Emission from the Geminga-Like Gamma-Ray Pulsar J1836+5925

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The detection of radio emission from the gamma-ray pulsar J1836+5925 is reported. Rare events of radio emission from this object have been recorded with the LPA radio telescope at the Pushchino Radio Astronomy Observatory. A two- or three-component integrated profile and very narrow individual pulses are a peculiarity of the radio emission from the pulsar J1836+5925. The presence of an interpulse is also possible. We have measured the dispersion measure, DM = 23 ± 1 pc cm−3, and estimated the distance to the pulsar, 1.5 kpc. The flux density and the lower limit on the spectral index have been estimated.

作者简介

V. Malofeev

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Moscow obl., 142290 Russia

Email: malofeev@prao.ru
Россия, Пущино

O. Malov

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Moscow obl., 142290 Russia

Email: malofeev@prao.ru
Россия, Пущино

D. Teplykh

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Moscow obl., 142290 Russia

Email: malofeev@prao.ru
Россия, Пущино

M. Timirkeeva

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Moscow obl., 142290 Russia

编辑信件的主要联系方式.
Email: malofeev@prao.ru
Россия, Пущино

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