Axial rotation of BY Dra-type stars and related objects
نویسندگان
چکیده
منابع مشابه
A–type stars: evolution, rotation and binarity
We discuss the internal structure of stars in the mass range 1.5 to 4M⊙ from the PMS to the subgiant phase with a particular emphasis on the convective core and the convective superficial layers. Different physical aspects are considered such as overshooting, treatment of convection, microscopic diffusion and rotation. Their influence on the internal structure and on the photospheric chemical a...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1990
ISSN: 0074-1809
DOI: 10.1017/s0074180900187716