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Fine structure of the red giant clump from Hipparcos data, and distance determinations based on its mean magnitude
Authors:  o Girardi,Martin A. T. Groenewegen,Achim Weiss,&   Maurizio Salaris
Affiliation:Max-Planck-Institut fu¨r Astrophysik, Karl-Schwarzschild-Straße 1, D-85740 Garching bei Mu¨nchen, Germany,;Astrophysics Research Institute, Liverpool John Moores University, Byrom Street, Liverpool L3 3AF
Abstract:
Keywords:stars: evolution    Hertzsprung–Russell (HR) diagram    solar neighbourhood    Galaxy: stellar content    galaxies: distances and redshifts    Magellanic Clouds
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