Absorption Line Spectroscopy is a spectroscopic method within stellar spectroscopy that identifies and analyzes the dark spectral lines formed when atoms or ions in a star's outer layers absorb specific wavelengths of light, distinguishing it from emission-based techniques by its reliance on the attenuation of continuous background radiation to infer elemental composition, temperature, and motion.
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Publications per year
2017–2026
196
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4.9K
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22
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Centre National de la Recherche Scientifique
Paris, France
48 h-index
308 publications
19.1K citations
Space Telescope Science Institute
Baltimore, United States
42 h-index
112 publications
6.9K citations
California Institute of Technology
Pasadena, United States
38 h-index
107 publications
11.9K citations
University of California, Santa Cruz
Santa Cruz, United States
35 h-index
74 publications
9.2K citations
Johns Hopkins University
Baltimore, United States
32 h-index
73 publications
5.9K citations
University of Arizona
Tucson, United States
31 h-index
82 publications
7.4K citations
Goddard Space Flight Center
Greenbelt, United States
31 h-index
95 publications
5.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
31 h-index
90 publications
5.1K citations
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- The Astrophysical Journal
ApJ · 503 publications · 30.5K citations
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- Monthly Notices of the Royal Astronomical Society
219 publications · 10.1K citations
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- Astronomy and Astrophysics
135 publications · 6.6K citations
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- The Astrophysical Journal Supplement Series
43 publications · 2.8K citations
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- The Astronomical Journal
AJ · 67 publications · 3.3K citations
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