The RW Aur microjet: Testing MHD disk wind models

被引：4

作者：

Dougados, C ^{[1
]}

Cabrit, S

Lopez-Martin, L

Garcia, P

O'Brien, D

机构：

[1] Observ Grenoble, Astrophys Lab, Grenoble, France

[2] Observ Paris, LERMA, Paris, France

[3] Univ Porto, P-4100 Oporto, Portugal

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2003年 / 287卷 / 1-4期

关键词：

star formation; mass-loss; RW Aur;

D O I：

10.1023/B:ASTR.0000006212.95943.a5

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We conduct a detailed comparison between the kinematics, morpology and excitation conditions of the RW Aur microjet on scales < 200 AU with predictions from stationary, self-similar, cold disk wind solutions. Implications for launching and ionization mechanisms of jets in young stars are discussed.

引用

页码：135 / 138

页数：4

共 14 条

[1]

Bacciotti F, 1999, ASTRON ASTROPHYS, V342, P717

[2] Hubble Space Telescope/STIS spectroscopy of the optical outflow from DG Tauri:: Indications for rotation in the initial jet channel [J].