Analysing Stellar Populations Using Isochrones

Details Analysing Stellar Populations Using Isochrones Analysing Stellar Populations Using Isochrones

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..182f&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Astronomy and Astrophysics

Astronomy

Galaxies: Haloes, Stars: Population Ii, Methods: Data Analysis, Hertzsprung-Russell (Hr) Diagram

Scientific paper

We present methods for analysing colour-magnitude diagrams, with particular emphasis on studies of the field halo stellar populations of nearby galaxies. Special consideration is made to the analysis of stars on the Red Giant Branch (RGB), and methods of obtaining metallicity distributions for old populations based on analysis of evolved sections of the Colour Magnitude Diagram (CMD).

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