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H2 Emission from External Galaxies

Published online by Cambridge University Press:  07 August 2017

Kimiaki Kawara
Kimiaki Kawara*
Affiliation:
National Astronomical Observatory Mitaka, Tokyo 181, Japan

Abstract

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2 μm spectroscopic observations by many authors have revealed significant rotation-vibrational H2 emission is widespread from starburst to bare nucleus galaxies. Near-IR H2 emission lines can arise from various excitation sources: UV radiation by hot stars, shock excitation by supernova remnants or AGN driven winds, and UV/X-ray radiation by an AGN. In this review recent data will be compared with such H2 excitation models.

Type
External Galaxies
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 103 - 107
Copyright
Copyright © Kluwer 1992 

References

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