Infrared properties of OH galaxies

Details Infrared properties of OH galaxies Infrared properties of OH galaxies

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...338..804b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 338, March 15, 1989, p. 804-811.

Astronomy and Astrophysics

Astronomy

87

Galaxies, Hydroxyl Emission, Infrared Astronomy, Interstellar Masers, Water Masers, Absorption Spectra, Emission Spectra, Interstellar Matter, Luminosity, Radiation Distribution

Scientific paper

The IR properties of OH megamasers are analyzed, emphasizing the
differences between the OH-emitting and OH-absorbing sources. A
quadratic L(OH)-L(IR) relationship rather than a linear one is found for
the observed megamasers. Such a relationship can be easily understood in
terms of a low-gain amplification model.

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