Flame evolution during type la supernovae and the deflagration phase in the gravitationally confined detonation scenario
- Author
- TOWNSLEY, D. M1 2 ; CALDER, A. C1 3 ; ASIDA, S. M4 ; SEITENZAHL, I. R2 5 ; PENG, F1 2 3 ; VLADIMIROVA, N3 ; LAMB, D. Q1 3 5 ; TRURAN, J. W1 2 3 5 6
[1] Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, United States
[2] Joint Institute for Nuclear Astrophysics, University of Chicago, Chicago, IL 60637, United States
[3] Center for Astrophysical Thermonuclear Flashes, University of Chicago, Chicago, IL 60637, United States
[4] Racah Institute of Physics, Hebrew University, Jerusalem 91904, Israel
[5] Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, United States
[6] Argonne National Laboratory, Argonne, IL 60439, United States - Source
The Astrophysical journal. 2007, Vol 668, Num 2, pp 1118-1131, 14 p ; 1 ; ref : 1/4 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- hydrodynamics nuclear reactions, nucleosynthesis, abundances supemovae: general white dwarfs
- Keyword (fr)
- Abondance Déflagration Détonation Naine blanche Nucléosynthèse Supernova
- Keyword (en)
- Abundance Deflagration Detonations White dwarf stars Nucleosynthesis Supernovae
- Keyword (es)
- Deflagración
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19187077
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1086/521013 
https://dx.doi.org/10.1086/521013
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