Galactic Ultraviolet Background
Galactic Ultraviolet Background is a component of diffuse ultraviolet radiation originating from within the Milky Way Galaxy, distinguished from extragalactic contributions by its association with stellar populations, hot interstellar gas, and dust-scattered starlight confined to the Galactic disk and halo.
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3.9K
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214
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118
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2017–2026
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Ewald Puchwein, Francesco Haardt, Martin G. Haehnelt et al. · Monthly Notices of the Royal Astronomical Society · 2019 · 176 citations · Full text
Natural Sciences, Astronomy, Physics +13
UV habitable zones around M stars
A. P. Buccino, Guillermo A. Lemarchand, P. J. D. Mauas · Icarus · 2007 · 117 citations · Full text
Natural Sciences, Astronomy, Physics +14
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118

Johns Hopkins University
Baltimore, United States
8 h-index
9 publications
233 citations

Space Telescope Science Institute
Baltimore, United States
6 h-index
13 publications
371 citations
University of Arizona
Tucson, United States
5 h-index
7 publications
672 citations

Towson University
Towson, United States
4 h-index
6 publications
148 citations
Indian Institute of Astrophysics
Bengaluru, India
4 h-index
4 publications
98 citations
Goddard Space Flight Center
Greenbelt, United States
3 h-index
7 publications
215 citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
3 h-index
3 publications
224 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
3 h-index
11 publications
193 citations
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ApJ · 38 publications · 1.6K citations
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14 publications · 1.5K citations
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AJ · 4 publications · 144 citations
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PASP · 2 publications · 36 citations
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2 publications · 26 citations
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