On the possibility of observing the double emission line feature of H 2 and HD from primordial molecular cloud cores

Monthly Notices of the Royal Astronomical Society

Volumn 339, Issue 4, 2003, Pages 1256-1264

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

^a KYOTO UNIVERSITY   (Japan)

^b UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Cosmology: Observations; Galaxies: Formation; Ism: Molecules; Submillimetre

Indexed keywords

STARS;

ATACAMA LARGE MILLIMETER ARRAYS; COSMOLOGY OBSERVATIONS; DOUBLE PEAK; EMISSION LINES; GALAXY FORMATIONS; ISM:MOLECULES; LINE FEATURES; MOLECULAR CLOUDS; ROTATIONAL TRANSITION; SUBMILLIMETRE;

CLOUDS;

EID: 0142137255     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06293.x     Document Type: Article

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