ISO observations of star-forming galaxies

被引：1

作者：

Mobasher, B ^{[1
]}

Afonso, J ^{[1
]}

Cram, L ^{[1
]}

机构：

[1] Space Telescope Sci Inst, Baltimore, MD 21218 USA

来源：

DEEP FIELDS | 2001年

关键词：

D O I：

10.1007/10854354_27

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Infrared Space Observatory (ISO) is used to carry out mid-IR (7 and 15 mum) and far-IR (90 mum) observations of a sample of star-forming sub-mJy radio sources. By selecting the sample at radio wavelengths, one avoids biases due to dust obscuration. It is found that the mid-IR luminosities, covering the PAH features, measure the star formation rate for galaxies with P-1.4GHz < 1023 W Hz(-1). This is further confirmed using the Halpha luminosities. The far-IR emission is also found to trace the SFR over the whole range of radio and Halpha luminosities. The implication of the mid-IR measurements in estimating the SFRs from the future infrared space missions (SIRTF and ASTRO-F) is discussed.

引用

页码：144 / 148

页数：5

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