NICMOS and WFPC2 imaging of ultraluminous galaxies

被引：0
|
作者：
Borne, KD [1 ]
Bushouse, H [1 ]
Colina, L [1 ]
Lucas, RA [1 ]
Baker, A [1 ]
Clements, D [1 ]
Lawrence, A [1 ]
Oliver, S [1 ]
Rowan-Robinson, M [1 ]
机构：
[1] NASA, Goddard Space Flight Ctr, Raytheon STX Corp, Greenbelt, MD 20771 USA
来源：
ASTROPHYSICS WITH INFRARED SURVEYS: A PRELUDE TO SIRTF | 1999年 / 177卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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.
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页码：167 / 170
页数：4
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