Star Formation In the Early Universe: The Collapse and Fragmentation of Zero Metal Gas

Details Star Formation In the Early Universe: The Collapse and Fragmentation of Zero Metal Gas Star Formation In the Early Universe: The Collapse and Fragmentation of Zero Metal Gas

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998baas...30r.762c&link_type=abstract

American Astronomical Society Meeting, 191, #127.01

Astronomy and Astrophysics

Astronomy

Scientific paper

We present preliminary results from three-dimensional simulations of the collapse and fragmentation of primordial, zero zero metallicity gas. Our long-term goal is to shed light on the characteristic mass scale of the first generation of stars. (Current estimates run the gamut, from ~ 1 to 10(5) solar masses.) The simulations are done using a special version of the TREESPH code, modified to include the appropriate chemistry and cooling function for primordial gas.

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