Thermal-chemical instability in a pre-galactic gas cloud

Details Thermal-chemical instability in a pre-galactic gas cloud Thermal-chemical instability in a pre-galactic gas cloud

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..167s&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Statistics

Computation

Cosmic Gases, Galactic Evolution, Gas Dynamics, Interstellar Chemistry, Thermal Stability, Computational Astrophysics, Condensing, Cosmochemistry, Stellar Mass, Temporal Distribution

Scientific paper

The growth of thermal-chemical instability in a pre-galactic medium is
followed by numerical simulation of gas dynamics. Results show that a
primordial gas cloud breaks into self-gravitating subcondensations with
the mass of normal stars.

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