White Dwarf Envelopes
White Dwarf Envelopes is a theoretical construct in astrophysics that denotes the outer layers of a white dwarf star, distinguished from other stellar envelope models by its application to degenerate, Earth-sized remnants composed primarily of electron-degenerate matter and characterized by extreme surface gravities and thin non-degenerate envelopes of hydrogen or helium.
191
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12K
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394
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199
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2017–2026
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Nucleosynthesis in Classical Novae: CO versus ONe White Dwarfs
J. José, M. Hernanz · The Astrophysical Journal · 1998 · 488 citations · Full text
Natural Sciences, Astronomy, Physics +15
A New Model for Progenitor Systems of Type Ia Supernovae
Izumi Hachisu, Mariko Kato, K. Nomoto · The Astrophysical Journal · 1996 · 475 citations · Full text
Natural Sciences, Astronomy, Physics +17
Diffusion coefficients for stellar plasmas
C. Paquette, C. Pelletier, G. Fontaine et al. · The Astrophysical Journal Supplement Series · 1986 · 378 citations
Natural Sciences, Astronomy, Physics +17
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Institut d'Estudis Espacials de Catalunya
Castelldefels, Spain
14 h-index
31 publications
2K citations
Universitat Politècnica de Catalunya
Barcelona, Spain
13 h-index
23 publications
1.3K citations

Universidad Nacional de La Plata
La Plata, Argentina
13 h-index
31 publications
1.9K citations

University of Warwick
Coventry, United Kingdom
10 h-index
26 publications
1.7K citations
University of Valparaíso
Valparaíso, Chile
9 h-index
23 publications
1.2K citations
University of Cambridge
Cambridge, United Kingdom
7 h-index
8 publications
270 citations
Institute of Astronomy
Moscow, Russia
7 h-index
11 publications
1.3K citations
The University of Tokyo
Tokyo, Japan
7 h-index
12 publications
2.1K citations
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ApJ · 83 publications · 5.8K citations
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46 publications · 3.1K citations
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17 publications · 921 citations
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5 publications · 636 citations
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Repository · 4 publications · 237 citations
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