Evolution and Spectrum of the Radio Emission of Tycho’s Supernova Remnant
- Авторлар: Vinyaikin E.N.1
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Мекемелер:
- Lobachevsky State University of Nizhny Novgorod (NNSU)
- Шығарылым: Том 62, № 2 (2018)
- Беттер: 130-137
- Бөлім: Article
- URL: https://ogarev-online.ru/1063-7729/article/view/191447
- DOI: https://doi.org/10.1134/S1063772918020063
- ID: 191447
Дәйексөз келтіру
Аннотация
The radio spectrum of Tycho’s Supernova Remnant is constructed at frequencies 12.6–143 000 MHz for epoch 2010.3, taking into account the secular decrease in the radio flux density of the remnant at the rate d = −(0.46 ± 0.03)%/year:
\(S_\nu ^{3C10} (t = 2010.3) = (43.1 \pm 1.8 Jy)(\nu [GHz])^{ - (0.592 \pm 0.019) + (0.041 \pm 0.012)\log (\nu [GHz])} .\)![]()
The spectrum has positive curvature. The presence of a low-frequency turnover in the spectrum of the radio source 3C10 with its maximum at 7.7 MHz is predicted, due to absorption in the interstellar medium in the direction toward the source.Авторлар туралы
E. Vinyaikin
Lobachevsky State University of Nizhny Novgorod (NNSU)
Хат алмасуға жауапты Автор.
Email: evin@nirfi.unn.ru
Ресей, Nizhny Novgorod, 603950
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