### 抜粋

We present a new formulation to compute numerically stationary and axisymmetric equilibria of magnetized and self-gravitating astrophysical fluids. Under the assumption of ideal MHD, the stream function for the flow can be chosen as a basic variable with which the Euler-Maxwell equations are cast into a set of basic equations, i.e. a generalized Bernoulli equation and a Grad-Shafranov-like equation by employing various integral conditions. A novel feature of this formulation is that systems with stars, disks and winds are treated in a simple unified picture and the magnetic field structures can contain both poloidal and toroidal components.

元の言語 | English |
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ホスト出版物のタイトル | Proceedings of the International Astronomical Union |

ページ | 437-440 |

ページ数 | 4 |

巻 | 6 |

エディション | S274 |

DOI | |

出版物ステータス | Published - 2010 9 |

外部発表 | Yes |

### 出版物シリーズ

名前 | Proceedings of the International Astronomical Union |
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番号 | S274 |

巻 | 6 |

ISSN（印刷物） | 17439213 |

ISSN（電子版） | 17439221 |

### ASJC Scopus subject areas

- Astronomy and Astrophysics

## フィンガープリント Stationary and axisymmetric magnetized equilibria of stars and winds' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。

## これを引用

*Proceedings of the International Astronomical Union*(S274 版, 巻 6, pp. 437-440). (Proceedings of the International Astronomical Union; 巻数 6, 番号 S274). https://doi.org/10.1017/S1743921311007435