ASTEROSEISMIC ANALYSIS OF THE INTERNAL STRUCTURE AND EVOLUTION OF RED GIANT BRANCH BUMP STARS

ABSTRACT The "bump" is a prominent feature of the red giant branch (RGB) luminosity function of stellar clusters. Through constructing a grid of models with different masses and metallicities to study the feature of the RGB bump luminosity we find that the luminosity increases almost monot...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 804; no. 1; pp. 6 - 10
Main Authors Gai, Ning, Tang, Yanke
Format Journal Article
LanguageEnglish
Published The American Astronomical Society 01.05.2015
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