Grids of stellar models IV (Schaerer+, 1993)

Details Grids of stellar models IV (Schaerer+, 1993) Grids of stellar models IV (Schaerer+, 1993)

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ycat..41020339s&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/102/339. Originally published in: 1993A&AS..102..339S

Physics

Models: Evolutionary, Mass Loss, Hr Diagrams

Scientific paper

The present grid of evolutionary sequences at metallicity Z=0.040, completes the set of grids computed for Z=0.020 and 0.001 by Schaller et al. (1992, Cat. J/A+AS/96/269), Z=0.008 by Schaerer et al. (1992, Cat. J/A+AS/98/523) and Z=0.004 by Charbonnel et al. (1993, Cat. J/A+AS/101/415). The models with mass loss and moderate core overshooting have been computed for 0.8 to 120 M&sun; using up-to-date input physics and the new radiative opacities from Iglesias et al. (1992ApJ...397..717I) and Kurucz (1991).
(22 data files).

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