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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 | Affiliation: | 1 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 | Abstract: | HST 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 | Services: | Forum | Review | PDF | Favorites |
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