Modelling binary stars: age, helium abundance and convection parameters-Reference-Cited by-同舟云学术

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Modelling binary stars: age, helium abundance and convection parameters

Published:2012-09-05 Issue:4 Volume:425 Page:3104-3111
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Fernandes J.¹,Vaz A. I. F.²,Vicente L. N.³

Affiliation:

1. CGUC; Department of Mathematics and Astronomical Observatory; University of Coimbra; Portugal

2. Algoritmi Centre and Department of Production and Systems; University of Minho; Portugal

3. CMUC; Department of Mathematics; University of Coimbra; Portugal

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/425/4/3104/4915520/425-4-3104.pdf

Reference54 articles.

1. Low-temperature Rosseland opacities

2. Accurate masses and radii of normal stars

3. On the Rotational Evolution of Solar‐ and Late‐Type Stars, Its Magnetic Origins, and the Possibility of Stellar Gyrochronology

4. Scaled solar tracks and isochrones in a large region of the Z–Y plane

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