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28 March 2024
 
  » arxiv » astro-ph/9809040

 Article overview


HST NICMOS and WFPC2 Imaging of Ultraluminous Galaxies
K. D. Borne ; H. Bushouse ; L. Colina ; R. A. Lucas ; A. Baker ; D. Clements ; A. Lawrence ; S. Oliver ; M. Rowan-Robinson ;
Date 3 Sep 1998
Subject astro-ph
Affiliation1 and 2), H. Bushouse , L. Colina (3 and 4), R. A. Lucas , A. Baker , D. Clements , A. Lawrence , S. Oliver , and M. Rowan-Robinson ( Raytheon STX, NASA GSFC, STScI, ESA, Saclay, IAS, IoA, Imperial College
AbstractHST 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.
Source arXiv, astro-ph/9809040
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