Структура аккреционного диска с облучением в тесных двойных системах с нейтронными звездами
Диссертация
Наряду с собственным нагревом из-за вязкости, аккреционный диск может поглощать и перерабатывать в тепло падающее на него излучение. В тесных двойных системах с релятивистским объектом (нейтронной звездой или черной дырой), мощным источником рентгеновского излучения являются центральные области диска. Часть рентгеновских фотонов может перехватываться внешними частями диска, поскольку аккреционный… Читать ещё >
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