Evolution of Mid-Mass Population III Stars

Details Evolution of Mid-Mass Population III Stars Evolution of Mid-Mass Population III Stars

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21542505l&link_type=abstract

American Astronomical Society, AAS Meeting #215, #425.05; Bulletin of the American Astronomical Society, Vol. 42, p.336

Astronomy and Astrophysics

Astronomy

Scientific paper

A growing body of work exists for theoretical, Population III (Pop III), stars. This is particularly true for very large mass evolution and low mass evolution. Less has been done for mid-mass Pop III stars in the range of 10 - 60 M. Though there is some consensus that the "first” stars were very massive, feedback from these may have induced the production of lower mass and middle mass stars also free of heavy elements. We present numerical evolution results for middle mass Pop III stars from pre-main sequence through to a core of Silicon. We further use our evolution models for numerical simulations of resulting supernovae light curves.

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