Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability
- Author
- 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 - Source
The Astrophysical journal. 2004, Vol 610, Num 2, pp 920-932, 13 p ; 1 ; ref : 45 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
- Russian
- Keyword (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
- Keyword (en)
- Magnetic fields Dipoles Accretion disks T Tauri stars Cataclysmic variable stars Three dimensional model MHD model Hot spots Millisecond pulsar Digital simulation Variability
- Keyword (es)
- Modelo 3 dimensiones Modelo MHD Pulsar milisegundo Variabilidad
- Classification
- 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
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 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
Access to the document
Install on your browser
DOI
10.1086/421867 
https://dx.doi.org/10.1086/421867
"O:13:\"PanistOpenUrl\":36:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000idc\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:14:\"10.1086\/421867\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2004\";s:9:\"\u0000*\u0000volume\";s:3:\"610\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"920\";s:8:\"\u0000*\u0000epage\";s:3:\"932\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"ROMANOVA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:3:{i:0;s:15:\"USTYUGOVA, G. V\";i:1;s:13:\"KOLDOBA, A. V\";i:2;s:17:\"LOVELACE, R. V. E\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:2:\"13\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Panist access
"O:12:\"IstexOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:14:\"10.1086\/421867\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2004\";s:9:\"\u0000*\u0000volume\";s:3:\"610\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"920\";s:8:\"\u0000*\u0000epage\";s:3:\"932\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"ROMANOVA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:3:{i:0;s:15:\"USTYUGOVA, G. V\";i:1;s:13:\"KOLDOBA, A. V\";i:2;s:17:\"LOVELACE, R. V. E\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:2:\"13\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Istex access
"O:16:\"UnpaywallOpenUrl\":35:{s:8:\"\u0000*\u0000email\";s:27:\"assistance-portail@inist.fr\";s:6:\"\u0000*\u0000fmt\";N;s:6:\"\u0000*\u0000doi\";s:14:\"10.1086\/421867\";s:6:\"\u0000*\u0000pii\";N;s:7:\"\u0000*\u0000pmid\";N;s:9:\"\u0000*\u0000atitle\";N;s:9:\"\u0000*\u0000jtitle\";N;s:9:\"\u0000*\u0000stitle\";N;s:7:\"\u0000*\u0000date\";N;s:9:\"\u0000*\u0000volume\";N;s:8:\"\u0000*\u0000issue\";N;s:8:\"\u0000*\u0000spage\";N;s:8:\"\u0000*\u0000epage\";N;s:8:\"\u0000*\u0000pages\";N;s:7:\"\u0000*\u0000issn\";N;s:8:\"\u0000*\u0000eissn\";N;s:9:\"\u0000*\u0000aulast\";N;s:10:\"\u0000*\u0000aufirst\";N;s:9:\"\u0000*\u0000auinit\";N;s:10:\"\u0000*\u0000auinitm\";N;s:5:\"\u0000*\u0000au\";N;s:9:\"\u0000*\u0000aucorp\";N;s:7:\"\u0000*\u0000isbn\";N;s:8:\"\u0000*\u0000coden\";N;s:8:\"\u0000*\u0000genre\";N;s:7:\"\u0000*\u0000part\";N;s:9:\"\u0000*\u0000btitle\";N;s:8:\"\u0000*\u0000title\";N;s:8:\"\u0000*\u0000place\";N;s:6:\"\u0000*\u0000pub\";N;s:10:\"\u0000*\u0000edition\";N;s:9:\"\u0000*\u0000tpages\";N;s:9:\"\u0000*\u0000series\";N;s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";N;}"
Unpaywall access
"O:16:\"EuropePMCOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:14:\"10.1086\/421867\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2004\";s:9:\"\u0000*\u0000volume\";s:3:\"610\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"920\";s:8:\"\u0000*\u0000epage\";s:3:\"932\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"ROMANOVA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:3:{i:0;s:15:\"USTYUGOVA, G. V\";i:1;s:13:\"KOLDOBA, A. V\";i:2;s:17:\"LOVELACE, R. V. E\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:2:\"13\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Europe PubMed Central access
"O:11:\"BaseOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:14:\"10.1086\/421867\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2004\";s:9:\"\u0000*\u0000volume\";s:3:\"610\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"920\";s:8:\"\u0000*\u0000epage\";s:3:\"932\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"ROMANOVA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:3:{i:0;s:15:\"USTYUGOVA, G. V\";i:1;s:13:\"KOLDOBA, A. V\";i:2;s:17:\"LOVELACE, R. V. E\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:2:\"13\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Base Search access
"O:12:\"ArXivOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:14:\"10.1086\/421867\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:9:\"\u0000*\u0000jtitle\";s:25:\"The Astrophysical journal\";s:9:\"\u0000*\u0000stitle\";s:12:\"Astrophys. j\";s:7:\"\u0000*\u0000date\";s:4:\"2004\";s:9:\"\u0000*\u0000volume\";s:3:\"610\";s:8:\"\u0000*\u0000issue\";s:1:\"2\";s:8:\"\u0000*\u0000spage\";s:3:\"920\";s:8:\"\u0000*\u0000epage\";s:3:\"932\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0004-637X\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"ROMANOVA\";s:10:\"\u0000*\u0000aufirst\";s:4:\"M. M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:3:{i:0;s:15:\"USTYUGOVA, G. V\";i:1;s:13:\"KOLDOBA, A. V\";i:2;s:17:\"LOVELACE, R. V. E\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"ASJOAB\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:1:\"1\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:100:\"Three-dimensional simulations of disk accretion to an inclined dipole. II: Hot spots and variability\";s:8:\"\u0000*\u0000place\";s:11:\"Chicago, IL\";s:6:\"\u0000*\u0000pub\";s:27:\"University of Chicago Press\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:2:\"13\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
arXiv access
