Rotation in Pre-Main Sequence Stars: Properties and Evolution
作者： J. Bouvier
DOI: 10.1007/978-94-011-3580-1_5
关键词: Circumstellar disk 、 T Tauri star 、 Accretion (astrophysics) 、 Physics 、 Stars 、 Rotation period 、 Main sequence 、 Astronomy 、 Angular momentum
摘要: The rotational properties of pre-main sequence stars with a mass between 0.5 and 9 M⊙ are reviewed. impact binarity disk accretion upon early evolution is discussed unsolved problems related to the stellar angular momentum prior main outlined.
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