A starburst origin of the OH-megamaser emission from the galaxy Arp220

The source of very large far-infrared luminosities of ultraluminous infrared galaxies remains controversial. The detection of a strong mid-infrared OH absorption line in the prototypical megamaser and ultraluminous galaxy Arp220 is discussed.

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Veröffentlicht in:Nature (London) 1997-04, Vol.386 (6624), p.472-474
Hauptverfasser: Skinner, C. J, Smith, H. A, Sturm, E, Barlow, M. J, Cohen, R. J, Stacey, G. J
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container_end_page 474
container_issue 6624
container_start_page 472
container_title Nature (London)
container_volume 386
creator Skinner, C. J
Smith, H. A
Sturm, E
Barlow, M. J
Cohen, R. J
Stacey, G. J
description The source of very large far-infrared luminosities of ultraluminous infrared galaxies remains controversial. The detection of a strong mid-infrared OH absorption line in the prototypical megamaser and ultraluminous galaxy Arp220 is discussed.
doi_str_mv 10.1038/386472a0
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subjects Astronomical observations
Astronomy
Earth, ocean, space
Exact sciences and technology
Far infrared (10-300 μm)
Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations
Infrared radiation
Interstellar masers
Interstellar medium (ism) and nebulae in external galaxies
Quasars. Active or peculiar galaxies, objects, and systems
Starburst galaxies and infrared excess galaxies
Stars & galaxies
Stellar systems. Galactic and extragalactic objects and systems. The universe
title A starburst origin of the OH-megamaser emission from the galaxy Arp220
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