Lyman Continuum Attenuation
Lyman Continuum Attenuation is a astrophysical phenomenon representing the reduction in intensity of far-ultraviolet photons below 912 Å due to absorption by neutral hydrogen and interstellar dust along the line of sight.
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8.9K
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472
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2017–2026
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Eight per cent leakage of Lyman continuum photons from a compact, star-forming dwarf galaxy
Y. I. Izotov, Ivana Orlitová, D. Schaerer et al. · Nature · 2016 · 283 citations · Full text
Natural Sciences, Astronomy, Physics +11
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Centre National de la Recherche Scientifique
Paris, France
17 h-index
25 publications
2K citations
University of Geneva
Geneva, Switzerland
14 h-index
46 publications
4.2K citations

University of Massachusetts Amherst
Amherst Center, United States
13 h-index
23 publications
1.8K citations

Space Telescope Science Institute
Baltimore, United States
12 h-index
26 publications
3.1K citations
Institut de Recherche en Astrophysique et Planétologie
Toulouse, France
10 h-index
11 publications
1.4K citations
Goddard Space Flight Center
Greenbelt, United States
10 h-index
15 publications
1.2K citations
University College London
London, United Kingdom
9 h-index
9 publications
431 citations

Johns Hopkins University
Baltimore, United States
8 h-index
16 publications
1.2K citations
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ApJ · 39 publications · 4K citations
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22 publications · 2K citations
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10 publications · 723 citations
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5 publications · 404 citations
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JGR · 4 publications · 86 citations
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