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
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20066333/pdf
Reference20 articles.
1. Tracing a Z-track in the M 31 X-ray binary RX J0042.6+4115
2. RX J0042.3+4115: A stellar mass black hole binary identified in M 31
3. Identifying a black hole X-ray transient in M 31 with XMM-Newton and Chandra
4. Disc precession in the M31 dipping X-ray binary Bo 158?
5. RX J0042.3+4115: a stellar mass black hole binary identified in M 31, and other papers
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1. XMM–Newton discovery of transient 285.4 s X-ray pulsar XMMU J013359.5+303634 in M33;Monthly Notices of the Royal Astronomical Society;2013-09-05
2. REINSTATING THE M31 X-RAY SYSTEM RX J0042.3+4115 AS A BLACK HOLE X-RAY BINARY AND COMPELLING EVIDENCE FOR AN EXTENDED CORONA;The Astrophysical Journal;2011-12-02
3. Challenging times: a re-analysis of NGC 5408 X-1;Monthly Notices of the Royal Astronomical Society;2010-10-29
4. In-depth studies of the NGC 253 ULXs withXMM-Newton: remarkable variability in ULX1, and evidence for extended coronae;Monthly Notices of the Royal Astronomical Society;2010-02
5. Low-metallicity natal environments and black hole masses in ultraluminous X-ray sources;Monthly Notices of the Royal Astronomical Society;2009-12-01
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