X-ray Novae
X-Ray Novae is a transient astrophysical phenomenon characterized by a sudden increase in X-ray emission from a compact binary system, distinguished from persistent X-ray sources by its episodic outburst behavior resulting from instabilities in the accretion disk around a stellar-mass black hole or neutron star.
227
Publications
10.4K
Citations
633
Authors
313
Institutions
Publications per year
2017–2026
24
Parents
227
The Properties of X‐Ray and Optical Light Curves of X‐Ray Novae
Wan Chen, C. R. Shrader, Mario Livio · The Astrophysical Journal · 1997 · 530 citations · Full text
Natural Sciences, Astronomy, Physics +14
The light curves of soft X-ray transients
A. R. King, H. G. Ritter · Monthly Notices of the Royal Astronomical Society · 1998 · 300 citations · Full text
Natural Sciences, Astronomy, Physics +12
1–5 of 227
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Center for Astrophysics Harvard & Smithsonian, United States
14 publications · 1.3K citations
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10
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10
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10
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Massachusetts Institute of Technology, United States
9 publications · 844 citations
9
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1–5 of 633
313
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
19 h-index
41 publications
3.2K citations

University of Leicester
Leicester, United Kingdom
19 h-index
52 publications
1.9K citations
Goddard Space Flight Center
Greenbelt, United States
18 h-index
36 publications
2.1K citations
The University of Tokyo
Tokyo, Japan
15 h-index
21 publications
548 citations
European Space Astronomy Centre
Madrid, Spain
14 h-index
29 publications
909 citations

Keio University
Tokyo, Japan
14 h-index
18 publications
478 citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
12 h-index
57 publications
3.2K citations
Deleted Institution
11 h-index
11 publications
290 citations
1–8 of 313
ApJ · 80 publications · 4.7K citations
37
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47 publications · 2.1K citations
25
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32 publications · 1.2K citations
20
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10 publications · 193 citations
10
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Repository · 5 publications · 140 citations
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