Hot cores:: probes of high-redshift galaxies?

被引：15

作者：

Lintott, CJ ^{[1
]}

Viti, S ^{[1
]}

Williams, DA ^{[1
]}

Rawlings, JMC ^{[1
]}

Ferreras, I ^{[1
]}

机构：

[1] UCL, Dept Phys & Astron, London WC1E 6BT, England

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2005年 / 360卷 / 04期

关键词：

astrochemistry; stars : formation; early Universe;

D O I：

10.1111/j.1365-2966.2005.09151.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 molecules in high-redshift hot cores should have detectable emission. It should be possible to distinguish between different models for the production of metals and hence hot core molecules should be useful probes of star formation at high redshift.

引用

页码：1527 / 1531

页数：5

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