Classical Novae
Classical Novae is a cataclysmic variable star phenomenon characterized by a sudden, dramatic increase in luminosity due to thermonuclear runaway of accreted hydrogen on the surface of a white dwarf in a close binary system.
360
Publications
15.7K
Citations
667
Authors
397
Institutions
Publications per year
2017–2026
64
360
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
Optically thick winds in nova outbursts
Mariko Kato, Izumi Hachisu · The Astrophysical Journal · 1994 · 276 citations
Natural Sciences, Astronomy, Physics +16
Michael M. Shara, Mario Livio, A. F. J. Moffat et al. · The Astrophysical Journal · 1986 · 240 citations
Natural Sciences, Astronomy, Physics +10
1–5 of 360
667
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397
Arizona State University
Tempe, United States
23 h-index
32 publications
1.7K citations
Universitat Politècnica de Catalunya
Barcelona, Spain
22 h-index
46 publications
2.2K citations
Institut d'Estudis Espacials de Catalunya
Castelldefels, Spain
22 h-index
55 publications
3.4K citations
Columbia University
New York, United States
19 h-index
44 publications
1.8K citations
Goddard Space Flight Center
Greenbelt, United States
18 h-index
29 publications
1.2K citations

University of Minnesota
Minneapolis, United States
17 h-index
42 publications
1.7K citations
Liverpool John Moores University
Liverpool, United Kingdom
16 h-index
48 publications
2.9K citations
The Ohio State University
Columbus, United States
16 h-index
35 publications
1.4K citations
1–8 of 397
ApJ · 126 publications · 6.9K citations
48
h-index
69 publications · 2.6K citations
28
h-index
43 publications · 1.7K citations
23
h-index
AJ · 15 publications · 472 citations
13
h-index
PASP · 10 publications · 727 citations
10
h-index
1–5