Low-metallicity Star Formation: the characteristic mass and upper mass limit

Details Low-metallicity Star Formation: the characteristic mass and upper mass limit Low-metallicity Star Formation: the characteristic mass and upper mass limit

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..255...49o&link_type=abstract

Low-Metallicity Star Formation: From the First Stars to Dwarf Galaxies, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

Stars: Formation, Stars: Population Ii

Scientific paper

We consider the fragmentation mass scale of low-metallicity clouds based
on their thermal evolution. Then we present the protostellar evolution
in the main accretion phase, and discuss the upper limit on the stellar
mass by the stellar feedback.

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