Numerical modeling of η carinae bipolar outflows
- Author
- GONZALEZ, R. F1 2 ; DE GOUVEIA DAL FINO, E. M2 ; RAGA, A. C1 ; VELAZQUEZ, P. F1
[1] Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Apartado Postal 70-543, 04510 México DF, Mexico
[2] Instituto Astronômico e Geofisico, Universidade de São Paulo, Rua do Matão 1226, 05508-090 São Paulo SP, Brazil - Source
The Astrophysical journal. 2004, Vol 616, Num 2, pp 976-987, 12 p ; 1 ; ref : 48 ref
- 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
- Keyword (fr)
- Ecoulement bipolaire Eruption stellaire Etoile massive Etoile variable bleue lumineuse Etoile variable éruptive Modèle 2 dimensions Modèle hydrodynamique Onde choc Simulation numérique Vent stellaire
- Keyword (en)
- Bipolar flow Stellar flares Massive stars Luminous blue variable star Eruptive variable stars Two dimensional model Hydrodynamic model Shock waves Digital simulation Stellar winds
- Keyword (es)
- Flujo bipolar Estrella variable azul luminosa Modelo 2 dimensiones
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10M Mass loss and stellar winds
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C30 Variable and peculiar stars (including novae) / 001E03C30E Emission-line stars (of, be, luminous blue variables, wolf-rayet, etc.)
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16357221
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
10.1086/425112 
https://dx.doi.org/10.1086/425112
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