SIMBAD references

2006MNRAS.368.1941Y - Mon. Not. R. Astron. Soc., 368, 1941-1948 (2006/June-1)

Modelling the components of binaries in the Hyades: the dependence of the mixing-length parameter on stellar mass.

YILDIZ M., YAKUT K., BAKIS H. and NOELS A.

Abstract (from CDS):

We present our findings based on a detailed analysis of the binaries of the Hyades, in which the masses of the components are well known. We fit the models of the components of a binary system to observations so as to give the observed total V and B-V of that system and the observed slope of the main sequence in the corresponding parts. According to our findings, there is a very definite relationship between the mixing-length parameter and the stellar mass. The fitting formula for this relationship can be given as α= 9.19(M/M- 0.74)0.053- 6.65, which is valid for stellar masses greater than 0.77M. While no strict information is gathered for the chemical composition of the cluster, as a result of degeneracy in the colour-magnitude diagram, by adopting Z= 0.033 and using models for the components of 70 Tau and θ2 Tau we find the hydrogen abundance to be X= 0.676 and the age to be 670 Myr. If we assume that Z= 0.024, then X= 0.718 and the age is 720 Myr. Our findings concerning the mixing-length parameter are valid for both sets of the solution. For both components of the active binary system V818 Tau, the differences between radii of the models with Z= 0.024 and the observed radii are only about 4 per cent. More generally, the effective temperatures of the models of low-mass stars in the binary systems studied are in good agreement with those determined by spectroscopic methods.

Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS

Journal keyword(s): stars: abundances - binaries: eclipsing - stars: evolution - stars: interiors - open clusters and associations: individual: Hyades

Simbad objects: 10

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2020.01.23-19:04:05

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