Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992)

Details Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992) Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992)

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ycat..40960269s&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/96/269. Originally published in: 1992A&AS...96..269S

Physics

Models: Evolutionary, Mass Loss, Stars: Supergiant, Stars: Wolf-Rayet

Scientific paper

New grids of stellar evolutionary models covering the range of 0.8 to 120 solar masses have been computed for metallicites Z=0.020 and Z=0.001. The models use the new opacities by Rogers and Iglesias (1992ApJS...79..507R) and by Kurucz (1991) at low T. The consequent changes in the solar helium content, in the mixing length ratio and in the overshooting parameter are taken into account after careful calibrations. Important physical ingredients as the nuclear reaction rates and the neutrino loss rates have been updated. The ionization of the main heavy elements is calculated in details. Results of the models are given in a compact way at corresponding evolutionary stages in each model. In addition to the tables, we shortly present some general results on the tracks in the HR diagrams, the lifetimes in the H-, He-, C-burning phases, and on massive and WR stars.
(50 data files).

Affiliated with

Also associated with

No associations

Rating

Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992) 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 Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1543689