Accretion of a clumped wind from a red supergiant donor on to a magnetar is suggested by the analysis of the XMM-Newton and NuSTAR observations of the X-ray binary 3A 1954+319

Author:

Bozzo, E.; Ferrigno, C.; Oskinova, L.; Ducci, L.

Tübinger Autor(en):

Published in:

Monthly Notices of The Royal Astronomical Society (2022), Bd. 510, H. 3, S. 4645-4653

Verlagsangabe:

Oxford Univ Press

Language:

English

Full text:

ISSN:

0035-8711

DDC Classifikation:

520 - Astronomy and allied sciences
530 - Physics

Dokumentart:

Article

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