Theoretical impact of fast rotation on calibrating the surface brightness-color relation for early-type stars-Reference-Cited by-同舟云学术

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Theoretical impact of fast rotation on calibrating the surface brightness-color relation for early-type stars

Published:2015-07 Issue: Volume:579 Page:A107
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Challouf M.,Nardetto N.,Domiciano de Souza A.,Mourard D.,Aroui H.,Stee P.,Delaa O.,Graczyk D.,Pietrzyński G.,Gieren W.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201526240/pdf

Reference50 articles.

1. Stellar Angular Diameters and Visual Surface Brightness -- I LATE SPECTRAL TYPES

2. Stellar Angular Diameters and Visual Surface Brightness -- II EARLY AND INTERMEDIATE SPECTRAL TYPES

3. Stellar angular diameters and visual surface brightness - III. An improved definition of the relationship

4. Cepheid distances from blue main-sequence companions

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