White Dwarf Evolution
White Dwarf Evolution is a theoretical framework within stellar astrophysics that describes the cooling and structural changes of white dwarfs over time as they radiate away residual thermal energy in the absence of nuclear fusion.
984
Publications
62.7K
Citations
1.5K
Authors
578
Institutions
Publications per year
2017–2026
208
984
Sub-Chandrasekhar mass models for Type IA supernovae
S. E. Woosley, T. A. Weaver · The Astrophysical Journal · 1994 · 566 citations
Natural Sciences, Astronomy, Physics +17
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578
Universitat Politècnica de Catalunya
Barcelona, Spain
43 h-index
157 publications
9.4K citations
Institut d'Estudis Espacials de Catalunya
Castelldefels, Spain
43 h-index
177 publications
11.9K citations

Universidad Nacional de La Plata
La Plata, Argentina
42 h-index
256 publications
15.5K citations

University of Warwick
Coventry, United Kingdom
40 h-index
174 publications
12.3K citations

Consejo Nacional de Investigaciones Científicas y Técnicas
Buenos Aires, Argentina
36 h-index
176 publications
11.4K citations
Instituto de Astrofísica de La Plata
La Plata, Argentina
29 h-index
134 publications
8.7K citations
Institute of Space Sciences
Cerdanyola del Vallès, Spain
26 h-index
46 publications
3.3K citations
Université de Montréal
Montreal, Canada
26 h-index
65 publications
6.9K citations
1–8 of 578
ApJ · 324 publications · 25.6K citations
83
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222 publications · 11.8K citations
61
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120 publications · 7.7K citations
46
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23 publications · 1K citations
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AJ · 16 publications · 562 citations
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