Journal article

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 independent 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 one thousand, then a wide range of molecules in high redshift hot cores should have detectable emission. It should be possible to distinguish between independent models for the production of metals and hence hot core molecules should be useful probes of star formation at high redshift.

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APA Style

Lintott, C., Viti, S., Williams, D., Rawlings, J., & Ferreras, I. (2005). Hot Cores : Probes of High-Redshift Galaxies. Monthly Notices of the Royal Astronomical Society, 360, 1527–1531.

MLA Style

Lintott, C, et al. “Hot Cores : Probes of High-Redshift Galaxies.” Monthly Notices of the Royal Astronomical Society, vol. 360, 2005, pp. 1527–31.

Chicago Style

Lintott, C, S Viti, D Williams, J Rawlings, and I Ferreras. 2005. “Hot Cores : Probes of High-Redshift Galaxies.” Monthly Notices of the Royal Astronomical Society 360: 1527–31.
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Publisher copy:: 10.1111/j.1365-2966.2005.09151.x

Authors

+ Lintott, C More by this author

Role:: Author

+ Viti, S More by this author

Role:: Author

+ Williams, D More by this author

Role:: Author

+ Rawlings, J More by this author

Role:: Author

+ Ferreras, I More by this author

Role:: Author

Journal:: Monthly Notices of the Royal Astronomical Society More from this journal
Volume:: 360
Pages:: 1527-1531
Publication date:: 2005-04-01
DOI:: 10.1111/j.1365-2966.2005.09151.x

Keywords:: astro-ph
Pubs id:: pubs:204330
UUID:: uuid:b8b4506d-8d41-41c0-a4bb-d8801b138d5c
Local pid:: pubs:204330
Source identifiers:: 204330
Deposit date:: 2012-12-19
ARK identifier:: ark:/29072/ora_b8b4506d8d4141c0a4bbd8801b138d5c

Terms of use

Copyright date:: 2005
Notes:: Updated to correspond to version accepted by MNRAS

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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