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Hot cores: Probes of high-redshift galaxies

Abstract:

The very high rates of second generation star formation detected and inferred in high-redshift objects should be accompanied by intense millimetre-wave emission from hot core molecules. We calculate the molecular abundances likely to arise in hot cores associated with massive star formation at high redshift, using several different models of metallicity in the early Universe. If the number of hot cores exceeds that in the Milky Way Galaxy by a factor of at least 1000, then a wide range of mol...

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Authors


Lintott, CJ More by this author
Williams, DA More by this author
Rawlings, JMC More by this author
Ferreras, I More by this author
Journal:
Monthly Notices of the Royal Astronomical Society
Volume:
360
Issue:
4
Pages:
1527-1531
Publication date:
2005-07-11
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:2af31360-cb1d-46e1-8646-405e146bc11c
Source identifiers:
159944
Local pid:
pubs:159944
Language:
English
Keywords:

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