Measurement of radio emission scattering parameters in the direction of pulsars B0809+74, B0919+06 and B1133+16 with ground-space interferometer RadioAstron
- Autores: Fadeev E.N.1, Andrianov A.S.1, Burgin M.S.1, Popov M.V.1, Rudnitskiy A.G.1, Smirnova T.V.1, Soglasnov V.A.1
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Afiliações:
- P. N. Lebedev Physical Institute of RAS
- Edição: Volume 101, Nº 11 (2024)
- Páginas: 986-1002
- Seção: Articles
- URL: https://cardiosomatics.ru/0004-6299/article/view/647678
- DOI: https://doi.org/10.31857/S0004629924110059
- EDN: https://elibrary.ru/JLGUER
- ID: 647678
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Resumo
We present the analysis of observations of three pulsars at a frequency of 327 MHz with the ground-space interferometer RadioAstron. The main scintillation parameters were measured: the decorrelation bandwidth ∆fdif and the scintillation time ∆tdif. We have found that these parameters vary significantly over time. For PSR B1133+16, the decorrelation bandwidth ∆fdif varied from 100 kHz to 350 kHz from 2014 to 2018. For PSR B0919+06 ∆fdif varied from 36 kHz to 195 kHz over approximately the same time period. In the direction of the observed pulsars, the power-law indices for the spatial inhomogeneity spectrum of the scattering plasma were estimated. The characteristic frequency and time scales of the diffractive scintillations for PSR B0809+74 are comparable to the receiver bandwidth and observation time, respectively. Therefore, only a lower limit for n can be obtained for this pulsar. For PSR B1133+16, the mean value is n = 3.40 ± 0.11, and n = 3.90 ± 0.04 for PSR B0919+06. We have also measured the angular diameter of the average scattering disks, θH , for these two pulsars. For PSR B0919+06, θH = 26 – 28 mas, and for B1133+16, θH = 12.0 ± 1.6 mas. We provide the estimates of the distance to the scattering screens. All measured parameters have been compared with previously published data.
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Sobre autores
E. Fadeev
P. N. Lebedev Physical Institute of RAS
Autor responsável pela correspondência
Email: fadeev@asc.rssi.ru
Astro-Space Center
Rússia, MoscowA. Andrianov
P. N. Lebedev Physical Institute of RAS
Email: fadeev@asc.rssi.ru
Astro-Space Center
Rússia, MoscowM. Burgin
P. N. Lebedev Physical Institute of RAS
Email: fadeev@asc.rssi.ru
Astro-Space Center
Rússia, MoscowM. Popov
P. N. Lebedev Physical Institute of RAS
Email: fadeev@asc.rssi.ru
Astro-Space Center
Rússia, MoscowA. Rudnitskiy
P. N. Lebedev Physical Institute of RAS
Email: fadeev@asc.rssi.ru
Astro-Space Center
Rússia, MoscowT. Smirnova
P. N. Lebedev Physical Institute of RAS
Email: fadeev@asc.rssi.ru
Puschino Radio Astronomical Observatory of the Astro-Space Center
Rússia, PuschinoV. Soglasnov
P. N. Lebedev Physical Institute of RAS
Email: fadeev@asc.rssi.ru
Astro-Space Center
Rússia, MoscowBibliografia
- N. W. Broten, J. L. Locke, T. H. Legg, C. W. McLeish, and R. S. Richards, Nature (London) 215(5096), 38 (1967).
- Н. С. Кардашев, А. В. Алакоз, А. С. Андрианов, М. И. Ар- тюхов, и др., Вестник НПО им. С. А. Лавочкина, № 3(33), p. 4 (2016), https://elibrary.ru/download/ elibrary_26421217_17562386.pdf .
- Н. С. Кардашев, А. В. Алакоз, А. С. Андрианов, У. Баан, и др., Вестник НПО им. С. А. Лавочкина, № 3(41), p. 3 (2018), https://elibrary.ru/download/elibrary_ 36328394_55227639.pdf .
- C. R. Gwinn, M. V. Popov, N. Bartel, A. S. Andrianov, et al., Astrophys. J. 822(2), id. 96 (2016), arXiv:1501.04449 [astro-ph.GA].
- M. V. Popov, N. Bartel, C. R. Gwinn, M. D. Johnson, et al., Monthly Not. Roy. Astron. Soc. 465(1), 978 (2017), arXiv:1609.04008 [astro-ph.HE].
- М. В. Попов, А. С. Андрианов, М. С. Бургин, В. А. Зуга, А. Г. Рудницкий, Т. В. Смирнова, В. А. Согласнов, Е. Н. Фа деев, Астрон. журн. 96(5), 393 (2019).
- T. V. Smirnova, V. I. Shishov, A. S. Andrianov, M. S. Burgin, et al., Monthly Not. Roy. Astron. Soc. 496(4), 5149 (2020).
- N. Bartel, M. S. Burgin, E. N. Fadeev, M. V. Popov, N. Ronaghikhameneh, T. V. Smirnova, and V. A. Soglasnov, Astrophys. J. 941(2), id. 112 (2022), arXiv:2210.16669 [astro-ph.GA].
- T. V. Smirnova, V. I. Shishov, M. V. Popov, C. R. Gwinn, et al., Astrophys. J. 786(2), id. 115 (2014), arXiv:1402.6346 [astro-ph.GA].
- 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), arXiv:1605.05727 [astro-ph.SR] .
- А. С. Андрианов, Т. В. Смирнова, В. И. Шишов, К. Гвин, М. В. Попов, Астрон. журн. 94(6), 516 (2017).
- М. В. Попов, А. С. Андрианов, Н. Бартель, К. Гвинн, и др., Астрон. журн. 93(9), 778 (2016).
- E. N. Fadeev, A. S. Andrianov, M. S. Burgin, M. V. Popov, A. G. Rudnitskiy, V. I. Shishov, T. V. Smirnova, and V. A. Zuga, Monthly Not. Roy. Astron. Soc. 480(3), 4199 (2018), arXiv:1801.06099 [astro-ph.GA].
- E. N. Fadeev, Res. Astron. and Astrophys. 18(8), id. 103 (2018), arXiv:1805.07983 [astro-ph.GA].
- М. В. Попов, Т. В. Смирнова, Астрон. журн. 98(11), 929 (2021).
- М. В. Попов, Астрон. журн. 99(12), 1264 (2022).
- V. I. Shishov, T. V. Smirnova, W. Sieber, V. M. Malofeev, et al., Astron. and Astrophys. 404(2), 557 (2003).
- C. R. Gwinn, J. M. Cordes, N. Bartel, A. Wolszczan, and R. L. Mutel, Astrophys. J. 334, L13 (1988).
- M. C. Britton, C. R. Gwinn, and M. J. Ojeda, Astrophys. J. 501, L101 (1998), arXiv:astro-ph/9610028.
- W. F. Brisken, J. M. Benson, W. M. Goss, and S. E. Thorsett, Astrophys. J. 571(2), 906 (2002), arXiv:astro-ph/0204105.
- S. Chatterjee, J. M. Cordes, T. J. W. Lazio, W. M. Goss, E. B. Fomalont, and J. M. Benson, Astrophys. J. 550(1), 287 (2001), arXiv:astro-ph/0010060.
- R. S. McGary, W. F. Brisken, A. S. Fruchter, W. M. Goss, and S. E. Thorsett, Astron. J. 121(2), 1192 (2001), arXiv:astro-ph/0010374.
- W. F. Brisken, J. P. Macquart, J. J. Gao, B. J. Rickett, W. A. Coles, A. T. Deller, S. J. Tingay, and C. J. West, Astrophys. J. 708(1), 232 (2010), arXiv:0910.5654 [astro-ph.GA].
- J. W. McKee, H. Zhu, D. R. Stinebring, and J. M. Cordes, Astrophys. J. 927(1), id. 99 (2022), arXiv:2112.11980 [astro-ph.HE].
- Т. В. Смирнова, В. И. Шишов, Астрон. журн. 85(9), 818 (2008).
- J. M. Cordes, J. M. Weisberg, and V. Boriakoff, Astrophys. J. 288, 221 (1985).
- J. M. Cordes and A. Wolszczan, Astrophys. J. 307, L27 (1986).
- N. D. R. Bhat, A. P. Rao, and Y. Gupta, Astrophys. J. Suppl. 121(2), 483 (1999), arXiv:astro-ph/9810354.
- J. M. Cordes and B. J. Rickett, Astrophys. J. 507(2), 846 (1998).
- J. A. Phillips and A. Wolszczan, Astrophys. J. 385, 273 (1992).
- D. R. Stinebring, M. A. McLaughlin, J. M. Cordes, K. M. Becker, J. E. E. Goodman, M. A. Kramer, J. L. Sheckard, and C. T. Smith, Astrophys. J. 549(1), L97 (2001), arXiv:astro-ph/0010363.
- M. A. Walker, D. B. Melrose, D. R. Stinebring, and C. M. Zhang, Monthly Not. Roy. Astron. Soc. 354(1), 43 (2004), arXiv:astro-ph/0403587.
- J. M. Cordes, B. J. Rickett, D. R. Stinebring, and W. A. Coles, Astrophys. J. 637(1), 346 (2006), arXiv:astro-ph/0407072.
- M. L. Putney and D. R. Stinebring, Chin. J. Astron. and Astrophys. Suppl. 6(S2), 233 (2006).
- A. S. Hill, D. R. Stinebring, C. T. Asplund, D. E. Berwick, W. B. Everett, and N. R. Hinkel, Astrophys. J. 619(2), L171 (2005), arXiv:astro-ph/0411752.
- D. R. Stinebring, Chin. J. Astron. and Astrophys. Suppl. 6(S2), 204 (2006).
- D. Stinebring, Astron. Astrophys. Trans. 26(6), 517 (2007).
- D. R. Stinebring, B. J. Rickett, and S. K. Ocker, Astrophys. J. 870(2), id. 82 (2019), arXiv:1811.04519 [astro-ph.GA].
- F. S. Trang and B. J. Rickett, Astrophys. J. 661(2), 1064 (2007), arXiv:astro-ph/0702210.
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