Interstellar scintillation of sources B0821+394 and B1812+412 according to observations on the LPA LPI radio telescope

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The search for long-term variability of compact components of radio sources B0821+394 and B1812+412 over an interval of 10 years was carried out. The LPA LPI radio telescope with an operating frequency of 111 MHz was used for observations. According to our estimates, the characteristic time of variability for both sources is 1.5–2.5 years. It is shown that the observed variability is not related to intrinsic variations in the radiation flux, but is due to refractive scintillation on inhomogeneities of the interstellar medium. From the obtained upper estimates of the apparent angular dimensions of the sources, it follows that the main contribution to the scattering of radio emission is made by turbulent plasma concentrated in sufficiently thin screens, the distance to which does not exceed 300–400 pc.

作者简介

S. Tyul'bashev

Lebedev Physical Institute

编辑信件的主要联系方式.
Email: serg@prao.ru

Astrospace center, Pushchino radio astronomy observatory

俄罗斯联邦, Pushchino, Moscow region

I. Chashei

Lebedev Physical Institute

Email: serg@prao.ru

Astrospace center, Pushchino radio astronomy observatory

俄罗斯联邦, Pushchino, Moscow region

I. Grishanova

Pushchino brunch of Russian Biotechnological University (Rosbiotech)

Email: serg@prao.ru
俄罗斯联邦, Pushchino, Moscow region

G. Tyul'basheva

Institute of Mathematical Problems of Biology RAS (IMPB RAS) brunch of Keldysh Institute of Applied Mathematics of Russian Academy of Sciences

Email: serg@prao.ru
俄罗斯联邦, Pushchino, Moscow region

I. Subaev

Lebedev Physical Institute

Email: serg@prao.ru

Astrospace center, Pushchino radio astronomy observatory

俄罗斯联邦, Pushchino, Moscow region

参考

  1. R. W. Hunstead, Astrophys. Letters 12, 193 (1972).
  2. W. D. Cotton, Astrophys. J. Suppl. 32, 467 (1976).
  3. C. Fanti, R. Fanti, A. Ficarra, F. Mantovani, L. Padrielli, and K. W. Weiler, Astron. and Astrophys. Suppl. Ser. 45, 61 (1981).
  4. O. B. Slee, Monthly Not. Roy. Astron. Soc. 235, 1313 (1988).
  5. M. M. McGilchrist and J. M. Riley, Monthly Not. Roy. Astron. Soc. 246, 123 (1990).
  6. I. S. Shklovsky, Nature 206, 176 (1965).
  7. H. van der Laan, Nature 211, 1131 (1966).
  8. A. P. Marscher and W. K. Gear, 298, 114 (1985).
  9. K. J. Mitchell, B. Dennison, J. J. Condon, D. R. Altschuler, H. E. Payne, S. L. O'Dell, and J. J. Broderick, Astrophys. J. Suppl. 93, 441 (1994).
  10. N. Ya. Shapirovskaya, Soviet Astron. 22, 544 (1978).
  11. B. J. Rickett, 307, 564 (1986).
  12. S. A. Tyul'bashev, P. Yu. Golysheva, V. S. Tyul'bashev, and I. A. Subaev, Astron. Rep. 63(11), 920 (2019).
  13. S. A. Tyul'Bashev and P. Augusto, Astron. and Astrophys. 439(3), 963 (2005).
  14. Y. Y. Kovalev, K. I. Kellermann, M. L. Lister, D. C. Homan, et al., Astran. J. 130(6), 2473 (2005).
  15. V. S. Artyukh and T. V. Smirnova, Soviet Astron. Letters 15(5), 344 (1989).
  16. B. J. Rickett, Ann. Rev. Astron. Astrophys. 28, 561 (1990).
  17. F. Mantovani, R. Fanti, L. Gregorini, L. Padrielli, and S. Spangler, Astron. and Astrophys. 233, 535 (1990).
  18. T. V. Smirnova, V. I. Shishov, M. V. Popov, C. R. Gwinn, et al., 786(2), id. 115 (2014).
  19. V. I. Shishov, T. V. Smirnova, C. R. Gwinn, A. S. Andrianov, M. V. Popov, A. G. Rudnitskiy, and V. A. Soglasnov, Monthly Not. Roy. Astron. Soc. 468(3), 3709 (2017).
  20. S. V. Pilipenko, Y. Y. Kovalev, A. S. Andrianov, U. Bach, et al., Monthly Not. Roy. Astron. Soc. 474(3), 3523 (2018).
  21. M. L. Lister, M. F. Aller, H. D. Aller, D. C. Homan, et al., Astron. J. 146(5), id. 120 (2013).
  22. D. R. Henstock, I. W. A. Browne, P. N. Wilkinson, G. B. Tay -lor, R. C. Vermeulen, T. J. Pearson, and A. C. S. Readhead, Astrophys. J. Suppl. 100, 1 (1995).

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