Period–luminosity relations of fast-rotating B-type stars in the young open cluster NGC 3766-Reference-Cited by-同舟云学术

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Period–luminosity relations of fast-rotating B-type stars in the young open cluster NGC 3766

Published:2017-02-11 Issue:4 Volume:467 Page:3864-3873
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Saio H.,Ekström S.,Mowlavi N.,Georgy C.,Saesen S.,Eggenberger P.,Semaan T.,Salmon S. J. A. J.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/467/4/3864/10907727/stx346.pdf

Reference56 articles.

1. Open clusters

2. On the effect of rotation on populations of classical Cepheids

3. Stability of g modes in rotating B-type stars

4. Updated opacities from the Opacity Project

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