Interstellar Emission Lines
Interstellar Emission Lines is a spectroscopic phenomenon consisting of discrete wavelengths of electromagnetic radiation emitted by ions, atoms, or molecules in the interstellar medium as they transition from higher to lower energy states, distinguishing it from absorption or continuum processes by its origin in spontaneous radiative transitions within low-density cosmic gases.
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Rest-Frame Ultraviolet Spectra of z~3 Lyman Break Galaxies
Alice E. Shapley, Charles C. Steidel, Max Pettini et al. · ArXiv.org · 2003 · 838 citations · Full text
Natural Sciences, Astronomy, Physics +13
The Diffuse Interstellar Bands
G. H. Herbig · Annual Review of Astronomy and Astrophysics · 1995 · 733 citations
Natural Sciences, Astronomy, Physics +10
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Space Telescope Science Institute
Baltimore, United States
46 h-index
154 publications
12K citations
California Institute of Technology
Pasadena, United States
38 h-index
113 publications
13.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
36 h-index
114 publications
10.5K citations

Centre National de la Recherche Scientifique
Paris, France
32 h-index
151 publications
12.4K citations
Goddard Space Flight Center
Greenbelt, United States
32 h-index
124 publications
10.5K citations
University of California, Berkeley
Berkeley, United States
31 h-index
116 publications
7.7K citations
University of Arizona
Tucson, United States
30 h-index
114 publications
13.9K citations

Johns Hopkins University
Baltimore, United States
30 h-index
101 publications
6.8K citations
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ApJ · 452 publications · 27.6K citations
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135 publications · 6.2K citations
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105 publications · 6K citations
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AJ · 47 publications · 2.9K citations
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