On the possibility of observing H2 emission from primordial molecular cloud kernels

Monthly Notices of the Royal Astronomical Society

Volumn 332, Issue 1, 2002, Pages 251-256

  Kamaya, Hideyuki ^a,b   Silk, Joseph ^a  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b KYOTO UNIVERSITY   (Japan)

Author keywords

Cosmology: observations; Galaxies: formation; Infrared: galaxies; ISM: molecules; Submillimetre

Indexed keywords

CLOUDS;

ACCRETION RATE; COSMOLOGY OBSERVATIONS; GALAXY FORMATIONS; INFRARED GALAXIES; ISM:MOLECULES; LINE RADIATION; MOLECULAR CLOUDS; RED SHIFT; SINGLE KERNEL; SUBMILLIMETRE;

STARS;

EID: 0041758468     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05301.x     Document Type: Article

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