(Q57867290)

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Disentangling discrepancies between stellar evolution theory and sub-solar mass stars. The influence of the mixing length parameter for the UV Psc binary

scientific article published in Astronomy and Astrophysics

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Disentangling discrepancies between stellar evolution theory and sub-solar mass stars. The influence of the mixing length parameter for the UV Psc binary (English)

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object named as

J. Fernandes

2

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author name string

E. Lastennet

1

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D. Valls-Gabaud

3

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E. Oblak

4

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language of work or name

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publication date

October 2003

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Astronomy and Astrophysics

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409

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2

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611–618

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Approximations to the radii of Roche lobes

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Updated Opal Opacities

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Constraining the difference in convective blueshift between the components of α Centauri with precise radial velocities

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Asteroseismology and calibration ofα Cen binary system

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Convective core mixing: A metallicity dependence?

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Low-temperature Rosseland opacities

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Detailed analysis of Balmer lines in cool dwarf stars

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A calibration of the 85 Peg binary system

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A comparison of stellar evolution with binary systems

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Detached double-lined eclipsing binaries as critical tests of stellar evolution age and metallicity determinations from the HR diagram

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The helium content and age of the Hyades: Constraints from five binary systems and Hipparcos parallaxes

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General properties of RS CVn systems

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The primordial helium abundance from observations of extragalactic HII regions

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Does the mixing length parameter depend on metallicity? Further tests of evolutionary sequences using homogeneous databases

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The chemical composition of the Small Magellanic Cloud H II region NGC 346 and the primordial helium abundance

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Further critical tests of stellar evolution by means of double-lined eclipsing binaries

1 reference

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Orbits of detached main-sequence eclipsing binaries of types late F to K. II. UV Leonis, UV Piscium, and BH Virginis

1 reference

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Hipparcos parallaxes of eclipsing binaries and the radiative flux scale

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Chemical composition of eclipsing binaries: a new approach to the helium-to-metal enrichment ratio

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Period changes in four short-period spotted binaries: UV Piscium, YY Geminorum, CG Cygni, and XY Ursae Majoris

1 reference

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The mixing length in convective stellar envelopes is proportional to distance from the convective boundary

1 reference

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Comparative seismology of pre- and main sequence stars in the instability strip

1 reference

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Consistent solar evolution model including diffusion and radiative acceleration effects

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Identifiers

10.1051/0004-6361:20031114

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2003A&A...409..611L

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astro-ph/0307360

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