Db White Dwarfs
DB White Dwarfs is a subclass of white dwarf stars characterized by a helium-dominated atmosphere with no detectable hydrogen, distinguished spectroscopically by the presence of neutral helium absorption lines in its optical spectrum.
207
Publications
11.6K
Citations
446
Authors
227
Institutions
Publications per year
2017–2026
30
Parents
207
S. J. Kleinman, S. O. Kepler, D. Koester et al. · The Astrophysical Journal Supplement Series · 2012 · 409 citations · Full text
Natural Sciences, Astronomy, Physics +17
A COMPREHENSIVE SPECTROSCOPIC ANALYSIS OF DB WHITE DWARFS
The Astrophysical Journal · 2011 · 355 citations · Full text
Natural Sciences, Astronomy, Physics +17
White dwarf mass distribution in the SDSS
Monthly Notices of the Royal Astronomical Society · 2007 · 327 citations · Full text
Natural Sciences, Astronomy, Physics +17
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227
Université de Montréal
Montreal, Canada
23 h-index
67 publications
5.7K citations
The University of Texas at Austin
Austin, United States
19 h-index
45 publications
3.6K citations

University of Warwick
Coventry, United Kingdom
16 h-index
54 publications
3.1K citations

Christian-Albrechts-Universität zu Kiel
Kiel, Germany
16 h-index
21 publications
2K citations
Universidade Federal do Rio Grande do Sul
Porto Alegre, Brazil
15 h-index
29 publications
3.7K citations

Universidad Nacional de La Plata
La Plata, Argentina
12 h-index
30 publications
1.9K citations
University of Arizona
Tucson, United States
11 h-index
20 publications
1.5K citations
University of Delaware
Newark, United States
9 h-index
16 publications
545 citations
1–8 of 227
ApJ · 88 publications · 5.1K citations
40
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38 publications · 1.5K citations
22
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25 publications · 1.5K citations
19
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AJ · 16 publications · 616 citations
14
h-index
10 publications · 1.2K citations
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