The Nature of Ultraluminous Infrared Galaxies

Details The Nature of Ultraluminous Infrared Galaxies The Nature of Ultraluminous Infrared Galaxies

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..204..179s&link_type=abstract

The Extragalactic Infrared Background and its Cosmological Implications, Proceedings of IAU Symposium #204, held 15-18 August 20

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The Infrared Space Observatory (ISO) has for the first time made possible mid- and far-infrared spectroscopic studies of nearby and moderate redshift, dusty ultraluminous infrared galaxies (ULIRGs). Recent SWS, LWS ISOPHOT-S and ISOCAM (CVF) results on ULIRGs will be discussed, along with high resolution ground-based near-IR and mm imaging spectroscopy. The following topics will be addressed: What powers ULIRGs? What is the AGN-starburst connection? How do ULIRGs evolve with time? What is the connection of the local ULIRG population to the recently discovered population of high redshift mid-IR to submm sources?

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