On the accretion flow geometry in A0535+26
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20010481/pdf
Reference31 articles.
1. Is GX5 – 1 a millisecond pulsar?
2. Accretion onto magnetized neutron stars - Structure and interchange instability of a model magnetosphere
3. Long-term variability of the Be/X-ray binary A 0535+26 -- I. Optical and UV spectroscopy
4. Infrared spectroscopy of the Be/X-ray transient A0535+26
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1. Awakening of the Fast-spinning Accreting Be/X-Ray Pulsar A0538–66;The Astrophysical Journal;2019-08-09
2. Magnetorotational instability in decretion disks of critically rotating stars and the outer structure of Be and Be/X-ray disks;Astronomy & Astrophysics;2014-12-09
3. Are There Magnetars in High‐Mass X‐Ray Binaries? The Case of Supergiant Fast X‐Ray Transients;The Astrophysical Journal;2008-08-20
4. Outbursts Large and Small from EXO 2030+375;The Astrophysical Journal;2008-05-10
5. HeI doubled emission lines from A0535+26 ≡ HDE 245770;Astronomy & Astrophysics;2007-06-18
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