Mixing-length parameter from binaries and clusters


Yildiz M.

252nd Symposium of the International-Astronomical-Union, Sanya, PEOPLES R CHINA, 6 - 11 Nisan 2008, ss.183-187 identifier identifier

  • Doi Numarası: 10.1017/s1743921308022734
  • Basıldığı Şehir: Sanya
  • Basıldığı Ülke: PEOPLES R CHINA
  • Sayfa Sayıları: ss.183-187

Özet

Mixing length parameter of the mixing length theory is a free parameter and used to calibrate radii of late-type stars. From the Hyades cluster and the alpha Centauri system, we find that the parameter depends on the stellar mass and some other properties of stars. Considering some other systems, we describe how the parameter depends on stellar parameters.