Galactic Flaring
Galactic Flaring is a phenomenon in galactic structure wherein the outer regions of a galaxy's disk exhibit an increase in vertical scale height with galactocentric radius, distinguishing it from uniform disk models by revealing a flared morphology due to variations in stellar or gas distribution.
41
Publications
2.8K
Citations
444
Authors
186
Institutions
Publications per year
2017–2026
11
Parents
41
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
1–5 of 41
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Max Planck Institute for Extraterrestrial Physics, Germany
2 publications · 69 citations
2
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2
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1–5 of 444
186
Instituto de Astrofísica de Canarias
Tenerife, Spain
5 h-index
8 publications
629 citations

Centre National de la Recherche Scientifique
Paris, France
4 h-index
58 publications
1K citations
Max Planck Institute for Astrophysics
Garching, Germany
4 h-index
7 publications
426 citations

University of Amsterdam
Amsterdam, The Netherlands
4 h-index
10 publications
170 citations
University of Michigan
Ann Arbor, United States
4 h-index
7 publications
394 citations
Université Paris Cité
Paris, France
3 h-index
30 publications
487 citations
California Institute of Technology
Pasadena, United States
3 h-index
5 publications
777 citations
Goddard Space Flight Center
Greenbelt, United States
3 h-index
4 publications
282 citations
1–8 of 186
ApJ · 12 publications · 739 citations
12
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9 publications · 617 citations
9
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4 publications · 239 citations
4
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3 publications · 722 citations
3
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2 publications · 124 citations
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