Galactic X-ray Background
The Galactic X-Ray Background is a diffuse astronomical phenomenon constituting a component of the X-ray background radiation that originates from within the Milky Way galaxy, primarily due to thermal emission from hot interstellar plasma and unresolved populations of X-ray-emitting stars and compact objects, thereby distinguishing it from extragalactic X-ray background sources.
327
Publications
21.3K
Citations
1.1K
Authors
316
Institutions
Publications per year
2017–2026
23
Variants
Galactic X-ray Background Radiation
Parents
327
Rapid X-ray flaring from the direction of the supermassive black hole at the Galactic Centre
Frederick K. Baganoff, M. W. Bautz, W. N. Brandt et al. · Nature · 2001 · 644 citations · Full text
Natural Sciences, Astronomy, Physics +16
X-ray background measurements with XMM-Newton EPIC
David H. Lumb, R. S. Warwick, M. J. Page et al. · Astronomy and Astrophysics · 2002 · 401 citations · Full text
Natural Sciences, Astronomy, Physics +17
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316
Goddard Space Flight Center
Greenbelt, United States
26 h-index
72 publications
4.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
24 h-index
74 publications
4K citations
Massachusetts Institute of Technology
Cambridge, United States
19 h-index
71 publications
4K citations

Space Research Institute
Moscow, Russia
19 h-index
63 publications
3.9K citations
Max Planck Institute for Astrophysics
Garching, Germany
18 h-index
46 publications
3.1K citations

Centre National de la Recherche Scientifique
Paris, France
15 h-index
36 publications
1.9K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
15 h-index
42 publications
4.7K citations
Institute of Space and Astronautical Science
Tokyo, Japan
15 h-index
43 publications
3.4K citations
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ApJ · 140 publications · 10K citations
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40 publications · 2.8K citations
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29 publications · 2.1K citations
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26 publications · 1.9K citations
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10 publications · 349 citations
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