Year: 2001
Type: article
Abstract: Thermal and chemical evolution of primordial gas clouds irradiated with far-ultraviolet (FUV; h ν < 13.6 eV) radiation is investigated. In clouds irradiated by intense FUV radiation, sufficient hydrogen molecules to be important for cooling are never formed. However, even without molecular hydrogen, if the clouds are massive enough, they start collapsing via atomic hydrogen line cooling. Such clouds continue to collapse almost isothermally owing to successive cooling by H - free-bound emission up to the number density of 10 16 cm -3 . Inside the clouds, the Jeans mass eventually falls well below a solar mass. This indicates that hydrogen molecules are dispensable for low-mass primordial star formation, provided that fragmentation of the clouds occurs at sufficiently high density.
Source: The Astrophysical Journal
DOI: 10.1086/318296
Author: Kazuyuki Omukai
Institution: National Astronomical Observatory of Japan
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W1998581888