NUMERICAL SIMULATIONS OF EQUATORIALLY ASYMMETRIC MAGNETIZED SUPERNOVAE : FORMATION OF MAGNETARS AND THEIR KICKS
- Author
- SAWAI, Hidetomo1 ; KOTAKE, Kei2 3 ; YAMADA, Shoichi1 4
[1] Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555, Japan
[2] Division of Theoretical Astronomy, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
[3] Max-Planck-Institute für Astrophysik, Karl-Schwarzshild-Strasse 1, 85741 Garching, Germany
[4] Advanced Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555, Japan - Source
The Astrophysical journal. 2008, Vol 672, Num 1, pp 465-478, 14 p ; 1 ; ref : 1/2 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
- MHD methods: numerical pulsars: general stars: magnetic fields; supernovae: general
- Keyword (fr)
- Champ magnétique Etoile magnétique Méthode numérique Pulsar Simulation numérique Supernova
- Keyword (en)
- Magnetic fields Magnetic stars Numerical method Pulsars Digital simulation Supernovae
- Keyword (es)
- Método numérico
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20002677
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
10.1086/523624 
https://dx.doi.org/10.1086/523624
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