PMS tracks at low Z for 0.1<=M<=1.5 (Di Criscienzo+, 2009)

Details PMS tracks at low Z for 0.1<=M<=1.5 (Di Criscienzo+, 2009) PMS tracks at low Z for 0.1<=M<=1.5 (Di Criscienzo+, 2009)

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..34960223d&link_type=abstract

VizieR On-line Data Catalog: J/A+A/496/223. Originally published in: 2009A&A...496..223D

Physics

Stars: Pre-Main Sequence, Models: Evolutionary

Scientific paper

We present pre-main-sequence (PMS) models for low mass stars from 0.1 to 1.5M_{sun} for metallicities [Fe/H]=-0.5, -1.0 and -2.0. The calculations include the most recent interior physics and the latest generation of non-grey atmosphere models. At fixed luminosity more metal poor isochrones are hotter than solar ones by {Delta}logTeff/{Delta}logZ~0.03-0.05 in the range in Z from 0.02 to 0.0002 and for ages from 105 to 107yr.
(2 data files).

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