Kelvin-Helmholtz instabilities as the source of inhomogeneous mixing in nova explosions
- Author
- CASANOVA, Jordi1 2 ; JOSE, Jordi1 2 ; ENRIQUE, García-Berro2 3 ; SHORE, Steven N4 ; CALDER, Alan C5
[1] Departament de Fisica i Enginyeria Nuclear, EUETIB, Universitat Politècnica de Catalunya, C./ Comte d'Urgell 187, 08036 Barcelona, Spain
[2] Institut d'Estudis Espacials de Catalunya, Ed. Nexus-201, C./ Gran Capita 2-4, 08034 Barcelona, Spain
[3] Departament de Fisica Aplicada, Universitat Politècnica de Catalunya, C./ Esteve Terrades 5, 08860 Castelldefels Barcelona, Spain
[4] Dipartimento di Fisica 'Enrico Fermi', Università di Pisa and Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Largo B. Pontecorvo 3, 56127 Pisa, Italy
[5] Department of Physics and Astronomy, Stony Brook University, Stony Brook, New York 11794-3800, United States - Source
Nature (London). 2011, Vol 478, Num 7370, pp 490-492, 3 p ; ref : 30 ref
- CODEN
- NATUAS
- ISSN
- 0028-0836
- Scientific domain
- Multidisciplinary
- Publisher
- Nature Publishing Group, London
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Keyword (fr)
- Abondance Explosion stellaire Gravité Instabilité Kelvin Helmholtz Matière interstellaire Modèle 3 dimensions Modèle hydrodynamique Mélangeage Métallicité Naine blanche Nova Simulation numérique Système stellaire Tourbillon
- Keyword (en)
- Abundance Stellar explosion Gravity Kelvin Helmholtz instability Interstellar matter Three dimensional model Hydrodynamic model Mixing Metallicity White dwarf stars Novae Digital simulation Stellar systems Vortices
- Keyword (es)
- Explosión estelar Inestabilidad Kelvin Helmholtz Modelo 3 dimensiones Metalicidad
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C30 Variable and peculiar stars (including novae) / 001E03C30Q Novae, dwarf novae, recurrent novae, and other cataclysmic (eruptive) variables
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 24636336
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
10.1038/nature10520 
https://dx.doi.org/10.1038/nature10520
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