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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Published in | The Astrophysical journal Vol. 804; no. 1; pp. 6 - 10 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
The American Astronomical Society
01.05.2015
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Subjects | |
Online Access | Get full text |
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