Theoretical isochrones for old, super-metal-rich stars

Details Theoretical isochrones for old, super-metal-rich stars Theoretical isochrones for old, super-metal-rich stars

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apjs...64..103v&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 64, May 1987, p. 103-125. NSERC-supported research.

Astronomy and Astrophysics

Astrophysics

106

Late Stars, Metallic Stars, Stellar Composition, Stellar Evolution, Galactic Structure, Star Distribution, Stellar Luminosity, Stellar Mass, Stellar Models

Scientific paper

A new and up-to-date set of theoretical evolutionary sequences and isochrones for super-metal-rich stars is presented. Models have been constructed for metallicities as high as Z = 0.10 and masses in the range of mass/solar mass = 0.6-1.5, in order to calculate isochrones for ages from 6 to 18 Gyr. The latest Los Alamos opacities are utilized, which have a pronounced effect on predicted mass-luminosity relations, and a value of 1.5 is adopted for the mixing-length parameter, which is required to reproduce the properties of the sun. The detailed numerical results are expected to be particularly useful in the construction of population synthesis models.

Affiliated with

Also associated with

No associations

Rating

Theoretical isochrones for old, super-metal-rich stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Theoretical isochrones for old, super-metal-rich stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theoretical isochrones for old, super-metal-rich stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-857185