Origin of magnetars in binary systemsстатья

Дата последнего поиска статьи во внешних источниках: 8 января 2017 г.

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[1] Popov S. B. Origin of magnetars in binary systems // Astronomical and Astrophysical Transactions. — 2016. — Vol. 29, no. 2. — P. 183–192. I review several scenarios of magnetar formation in binary systems via spin-up of a progenitor due to interaction with its companion. Mostly, these evolutionary channels lead to formation of isolated magnetars, and indeed, all well-established sources of this class are single objects. However, some binaries can survive, and several candidates to accreting magnetars have been proposed. I discuss this issue, and conclude that new accretion models can explain properties of the proposed candidates without large magnetic field in correspondence with models of magnetic field evolution.

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