MOShchNYE VSPLESKI I MAGNITOUPRUGIE KOLEBANIYa MAGNITAROV
- Autores: Yakovlev D.G.1
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Afiliações:
- Физико-технический институт им. А. Ф. Иоффе Российской академии наук
- Edição: Volume 166, Nº 1 (2024)
- Páginas: 121-132
- Seção: Articles
- URL: https://transsyst.ru/0044-4510/article/view/653859
- DOI: https://doi.org/10.31857/S0044451024070125
- ID: 653859
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Resumo
Магнитары — нейтронные звезды, обладающие сверхсильными магнитными полями, которые могут заметно превышать 1015 Гс. В некоторых из них (так называемых источниках мягких повторяющихся гамма-всплесков, soft gamma repeaters — SGRs) время от времени происходят процессы мощного энерговыделения, вызывающие необычайно сильные всплески электромагнитного излучения. Считается, что эти всплески связаны с наличием сверхсильных магнитных полей. Несмотря на множество гипотез, их механизм остается загадкой. В послесвечении всплесков выявлены квазипериодические осцилляции (КПО). Они трактуются как собственные колебания звезды, возбуждаемые при всплесках, и используются для диагностики всплесков. Показана существенная неполнота теорий, использованных для интерпретации КПО.Статья для специального выпуска ЖЭТФ, посвященного 130-летию П. Л. Капицы
Sobre autores
D. Yakovlev
Физико-технический институт им. А. Ф. Иоффе Российской академии наук
Email: yak.astro@mail.ioffe.ru
Санкт-Петербург, Россия
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