Mixing-length parameter from binaries and clusters

Details Mixing-length parameter from binaries and clusters Mixing-length parameter from binaries and clusters

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..252..183y&link_type=abstract

The Art of Modeling Stars in the 21st Century, Proceedings of the International Astronomical Union, IAU Symposium, Volume 252, p

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1

Convection, Stars: Interiors, Stars: Evolution, Stars: Late-Type, Binaries: Eclipsing, Stars: Individual (Α Cen, Fl Lyr, V442 Cyg)

Scientific paper

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 α 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.

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