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CO Observations of Ultraluminous Infrared Galaxies and Quasars

Published online by Cambridge University Press:  03 August 2017

D. B. Sanders
D. B. Sanders*
Affiliation:
Institute for Astronomy University of Hawaii 2680 Woodlawn Drive Honolulu, HI 96822

Abstract

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Recent millimeterwave observations of CO emission from ultraluminous infrared galaxies (Lir > 1012 L) and quasars suggest that abundant supplies of molecular gas may be a common property of both types of object. Current published CO detections are summarized, and the possibility of an evolutionary connection between infrared galaxies and quasars is discussed.

Type
XIII- IRAS Ultraluminous Objects and Quasars
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 417 - 424
Copyright
Copyright © Kluwer 1991 

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