Tables of theoretical isochrones for globular clusters

Details Tables of theoretical isochrones for globular clusters Tables of theoretical isochrones for globular clusters

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26as...36..429b&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 36, June 1979, p. 429-452. Research supported by the Consiglio Nazionale del

Astronomy and Astrophysics

Astrophysics

11

Chemical Composition, Globular Clusters, Isochromatics, Main Sequence Stars, Red Giant Stars, Stellar Evolution, Tables (Data), Astronomical Catalogs, Stellar Mass, Stellar Models

Scientific paper

Tables of isochrones are presented for stars in the core H-burning and shell H-burning phases, with mass in the range appropriate for globular clusters. Isochrones with age in the range 5 billion to 24 billion yr are presented for different sets of initial chemical composition. The isochrones were constructed by means of four networks of models with mass in the range 0.2-1.5 solar masses and evolved from the main sequence to the tip of the red giant branch.

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