The Diverse Population of ULIRGs

dc.creatorBorne, K. D.
dc.creatorArribas, S.
dc.creatorBushouse, H.
dc.creatorColina, L.
dc.creatorLucas, R. A.
dc.date2000-09-22
dc.date.accessioned2026-07-07T01:55:35Z
dc.date.available2026-07-07T01:55:35Z
dc.descriptionWe present results from an on-going Hubble Space Telescope (HST) survey of a large sample of ULIRGs (Ultra-Luminous IR Galaxies). New ground-based observations are now being used to complement the HST data and to assist in the interpretation of these complex objects. A rich spectroscopic, morphological, and dynamical diversity is found within the ULIRG population, nearly 100% of which are merger and/or collision remnants. The consequences of this diversity may apply to the interpretation of distant submm/FIR sources and their subsequent evolution.
dc.description3 pages. Paper to appear in the proceedings of the conference "FIRSED - Far-Infrared and Submillimeter Spectral Energy Distributions of Active and Starburst Galaxies", edited by I. van Bemmel, B. Wilkes, & P.Barthel, to be published in Elsevier New Astronomy Reviews
dc.identifierhttps://arxiv.org/abs/astro-ph/0009361
dc.identifierhttp://arxiv.org/abs/astro-ph/0009361
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1707
dc.subjectAstrophysics
dc.titleThe Diverse Population of ULIRGs
dc.typetext

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