RX J0042.3+4115: A stellar mass black hole binary identified in M 31
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20030638/pdf
Reference38 articles.
1. A Catalog and Atlas of Cataclysmic Variables: The Living Edition
2. Fender, R. 2002, in Relativistic Flows in Astrophysics, ed. A. W. Guthmann, M. Georganopoulos, A. Marcowith, & K. Manolakou, Lecture Notes in Physics, 589, 101
3. Frank, J., King, A. R., & Raine, D. 2002, Accretion Power in Astrophysics, 3rd Edition (Cambridge University Press)
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1. Fe Kα and Fe Kβ line detection in the NuSTAR spectrum of the ultra-bright Z source Scorpius X–1;Astronomy & Astrophysics;2021-10
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. NewXMM‐NewtonAnalysis of Three Bright X‐Ray Sources in M31 Globular Clusters, Including a New Black Hole Candidate;The Astrophysical Journal;2008-12-20
4. Time variability of X-ray sources in the M 31 centre field;Astronomy & Astrophysics;2008-01-17
5. 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;Astronomy & Astrophysics;2007-03-13
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