### Abstract

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.

Original language | English |
---|---|

Title of host publication | Proceedings of the International Astronomical Union |

Pages | 437-440 |

Number of pages | 4 |

Volume | 6 |

Edition | S274 |

DOIs | |

Publication status | Published - 2010 Sep |

Externally published | Yes |

### Publication series

Name | Proceedings of the International Astronomical Union |
---|---|

Number | S274 |

Volume | 6 |

ISSN (Print) | 17439213 |

ISSN (Electronic) | 17439221 |

### Fingerprint

### Keywords

- outflows
- stars: magnetic fields
- stars: rotation
- stars: winds

### ASJC Scopus subject areas

- Astronomy and Astrophysics

### Cite this

*Proceedings of the International Astronomical Union*(S274 ed., Vol. 6, pp. 437-440). (Proceedings of the International Astronomical Union; Vol. 6, No. S274). https://doi.org/10.1017/S1743921311007435

**Stationary and axisymmetric magnetized equilibria of stars and winds.** / Yoshida, Shin; Fujisawa, Kotaro; Eriguchi, Yoshiharu; Yoshida, Shijun; Takahashi, Rohta.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

*Proceedings of the International Astronomical Union.*S274 edn, vol. 6, Proceedings of the International Astronomical Union, no. S274, vol. 6, pp. 437-440. https://doi.org/10.1017/S1743921311007435

}

TY - GEN

T1 - Stationary and axisymmetric magnetized equilibria of stars and winds

AU - Yoshida, Shin

AU - Fujisawa, Kotaro

AU - Eriguchi, Yoshiharu

AU - Yoshida, Shijun

AU - Takahashi, Rohta

PY - 2010/9

Y1 - 2010/9

N2 - 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.

AB - 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.

KW - outflows

KW - stars: magnetic fields

KW - stars: rotation

KW - stars: winds

UR - http://www.scopus.com/inward/record.url?scp=79959277554&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=79959277554&partnerID=8YFLogxK

U2 - 10.1017/S1743921311007435

DO - 10.1017/S1743921311007435

M3 - Conference contribution

SN - 9780521197410

VL - 6

T3 - Proceedings of the International Astronomical Union

SP - 437

EP - 440

BT - Proceedings of the International Astronomical Union

ER -