Low-Metallicity Star Formation

Details Low-Metallicity Star Formation Low-Metallicity Star Formation

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1294..116o&link_type=abstract

THE FIRST STARS AND GALAXIES: CHALLENGES FOR THE NEXT DECADE. AIP Conference Proceedings, Volume 1294, pp. 116-121 (2010).

Physics

Star Formation, Population Iii Stars, Population Ii Main-Sequence Stars, Accretion, Stellar Mass, Star Formation, Population Iii Stars, Population Ii Stars, Accretion And Accretion Disks, Masses

Scientific paper

We study the evolution of low-metallicity star-forming clouds and discuss their fragmentation mass scales. From the structure of the envelope at the time of protostar formation, we derive the protostellar accretion rate and calculate the evolution of protostars in the main accretion phase. Finally, we evaluate the upper limit on the stellar mass set by stellar feedback.

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