Theoretical isochrones with convective overshoot

Details Theoretical isochrones with convective overshoot Theoretical isochrones with convective overshoot

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26as...85..845b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 85, no. 2, Oct. 1990, p. 845-853. Research supported by ASI.

Astronomy and Astrophysics

Astrophysics

86

Globular Clusters, Metallicity, Open Clusters, Stellar Evolution, Stellar Models, Charge Coupled Devices, Color-Magnitude Diagram, Magellanic Clouds, Milky Way Galaxy, Stellar Envelopes, Stellar Luminosity

Scientific paper

Theoretical isochrones for ages in the range from 20 Gyr to 40 Myr and various metallicities (Z = 0.0004, Z = 0.001, Z = 0.004, and Z = 0.020) are presented. These isochrones are derived from stellar models incorporating the effect of convective overshoot from the core, and include almost all evolutionary phases, starting from the main sequence to the stage of planetary nebula ejection, or carbon-ignition in a strongly electron degenerate carbon-oxygen core, or carbon-ignition in a mildly degenerate core, as appropriate according to the initial value of the mass. The isochrones also include the effect of mass loss by stationary wind and superwind.

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