Modelling the components of binaries in the Hyades: the dependence of the mixing-length parameter on stellar mass
Open Access
- 26 April 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 368 (4) , 1941-1948
- https://doi.org/10.1111/j.1365-2966.2006.10275.x
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This publication has 29 references indexed in Scilit:
- Line formation in solar granulationAstronomy & Astrophysics, 2004
- Oxygen trends in the Galactic thin and thick disksAstronomy & Astrophysics, 2004
- A Hipparcos study of the Hyades open clusterAstronomy & Astrophysics, 2001
- Stellar models and Hyades: the Hipparcos testMonthly Notices of the Royal Astronomical Society, 2001
- Callibration of stellar modelsThe Astrophysical Journal, 1995
- Low-temperature Rosseland opacitiesThe Astrophysical Journal, 1994
- Oxygen abundances in F-type stars of the Hyades and the Ursa Major groupThe Astrophysical Journal, 1993
- Thermonuclear reaction rates VAtomic Data and Nuclear Data Tables, 1988
- Carbon, nitrogen, and oxygen abundances in main-sequence stars. II 20 F and G starsThe Astrophysical Journal, 1981
- The value of the mixing lengthThe Astrophysical Journal, 1980