The nature of the interstellar medium of the starburst low-metallicity galaxy Haro 11: a multi-phase model of the infrared emission

Cormier, D.; Lebouteiller, V.; C. Madden, S.; Abel, N.; Hony, S.; Galliano, F.; Baes, M.; J. Barlow, M.; Cooray, A.; De Looze, I.; Galametz, M.; Ł. Karczewski, O.; J. Parkin, T.; Rémy, A.; Sauvage, M.; Spinoglio, L.; D. Wilson, C.; Wu, R.

doi:10.1051/0004-6361/201219818

Public

The nature of the interstellar medium of the starburst low-metallicity galaxy Haro 11: a multi-phase model of the infrared emission

Published in Astronomy and Astrophysics • Sep 7, 2012

Authors:

D. Cormier

V. Lebouteiller

S. C. Madden

Abstract

Context. The low-metallicity interstellar medium (ISM) is profoundly different from that of normal systems, being clumpy with low dust abundance and little CO-traced molecular gas. Yet many dwarf galaxies in the nearby universe are actively forming stars. As the complex ISM phases are spatially mixe...

Subject

Physics

Astrophysics

Interstellar medium

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