HST NICMOS and WFPC2 Imaging of Ultraluminous Galaxies

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dc.creatorBorne, K. D.
dc.creatorBushouse, H.
dc.creatorColina, L.
dc.creatorLucas, R. A.
dc.creatorBaker, A.
dc.creatorClements, D.
dc.creatorLawrence, A.
dc.creatorOliver, S.
dc.creatorRowan-Robinson, M.
dc.date1998-09-03
dc.date.accessioned2026-07-07T02:27:49Z
dc.date.available2026-07-07T02:27:49Z
dc.descriptionHST is used to study the power sources and the interaction-induced tidal disturbances within the most luminous galaxies in the local universe -- the Ultra-Luminous IR Galaxies (ULIRGs) -- through the use of I-band images with WFPC2 and H-band images with NICMOS. Such images are probing for the first time the fine-scale structures in the strong collision-disturbed morphologies of these rare and exotic galaxies.
dc.descriptionTo appear in "Astrophysics with Infrared Surveys: A Prelude to SIRTF," PASP Conference Proceedings, 4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9809040
dc.identifierhttp://arxiv.org/abs/astro-ph/9809040
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12855
dc.subjectAstrophysics
dc.titleHST NICMOS and WFPC2 Imaging of Ultraluminous Galaxies
dc.typetext

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