Sanders, D. B. and Soifer, B. T. and Scoville, N. Z. (1988) CO in infrared luminous galaxies. In: Molecular Clouds in the Milky Way and External Galaxies. Lecture Notes in Physics. No.315. Springer Berlin Heidelberg , Berlin, Heidelberg, pp. 350-360. ISBN 978-3-540-50438-2. https://resolver.caltech.edu/CaltechAUTHORS:20191008-073232893
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Abstract
There has been considerable recent interest in the properties of infrared galaxies due to the discovery by the Infrared Astronomical Satellite (IRAS) of a class of luminous galaxies which emit the bulk of their energy in the far-infrared (Houck et al. 1984; Soifer et al. 1984). Ground-based studies of these infrared luminous galaxies have shown that they are a substantial component of the local universe (z ~ 0.1) with a space density at luminosities above 1011 L⊙ (H_o = 75 km s^(-1)Mpc^(-1)) exceeding that of Seyfert galaxies and quasars (Soifer et al. 1986).
| Item Type: | Book Section | |||||||||
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| Additional Information: | © 1988 Springer-Verlag. | |||||||||
| Subject Keywords: | Star Formation; Spiral Galaxy; High Luminosity; Starburst Galaxy; Bright Galaxy | |||||||||
| Series Name: | Lecture Notes in Physics | |||||||||
| Issue or Number: | 315 | |||||||||
| DOI: | 10.1007/3-540-50438-9_302 | |||||||||
| Record Number: | CaltechAUTHORS:20191008-073232893 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20191008-073232893 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 99131 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 08 Oct 2019 16:39 | |||||||||
| Last Modified: | 16 Nov 2021 17:43 |
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