XMM–Newton discovery of transient 285.4 s X-ray pulsar XMMU J013359.5+303634 in M33
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/435/4/3326/3438964/stt1518.pdf
Reference42 articles.
1. Constraining compactness and magnetic field geometry of X-ray pulsars from the statistics of their pulse profiles
2. On the artificial nature of aperiodic variability in XMM-Newton observations of M 31 X-ray sources and the ultraluminous X-ray source NGC 4559 ULX-7
3. The Limiting Luminosity of Accreting Neutron Stars With Magnetic Fields
4. Observations of Accreting Pulsars
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1. Young Black Hole and Neutron Star Systems in the Nearby Star-forming Galaxy M33: The NuSTAR View;The Astrophysical Journal;2022-05-01
2. Using High-Mass X-ray binaries to probe massive binary evolution: The age distribution of High-Mass X-ray binaries in M33;Proceedings of the International Astronomical Union;2018-08
3. A DEEP XMM-NEWTON SURVEY OF M33: POINT-SOURCE CATALOG, SOURCE DETECTION, AND CHARACTERIZATION OF OVERLAPPING FIELDS;The Astrophysical Journal Supplement Series;2015-05-15
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