Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability
- Autor
- ROMANOVA, M. M1 ; USTYUGOVA, G. V2 ; KOLDOBA, A. V3 ; LOVELACE, R. V. E4
[1] Department of Astronomy, Cornell University, 410 Space Sciences Building, Ithaca, NY 14853-6801, United States
[2] Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, 4 Miusskaya Square, Moscow 125047, Russian Federation
[3] Institute of Mathematical Modeling, Russian Academy of Sciences, 4 Miusskaya Square, Moscow 125047, Russian Federation
[4] Department of Astronomy, Cornell University, 412 Space Sciences Building, Ithaca, NY 14853-6801, United States - Fuente
The Astrophysical journal. 2004, Vol 610, Num 2, pp 920-932, 13 p ; 1 ; ref : 45 ref
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- University of Chicago Press, Chicago, IL
- País de la publicación
- United States
- Tipo de documento
- Article
- Idioma
- Russian
- Palabra clave (fr)
- Champ magnétique Dipôle Disque accrétion Etoile type T Tauri Etoile variable cataclysmique Modèle 3 dimensions Modèle MHD Point chaud Pulsar milliseconde Simulation numérique Variabilité
- Palabra clave (in)
- Magnetic fields Dipoles Accretion disks T Tauri stars Cataclysmic variable stars Three dimensional model MHD model Hot spots Millisecond pulsar Digital simulation Variability
- Palabra clave (es)
- Modelo 3 dimensiones Modelo MHD Pulsar milisegundo Variabilidad
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10L Magnetic and electric fields. Polarization of starlight
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 15997786
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
10.1086/421867 
https://dx.doi.org/10.1086/421867
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