Published 2006
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Spitzer Mid-Infrared Imaging of Nearby Ultraluminous Infrared Galaxies
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Abstract
We have observed 14 nearby (z < 0.16) Ultraluminous Infrared Galaxies (ULIRGs) with Spitzer at 3.6-24μm. The underlying host galaxies are well-detected, in addition to the luminous nuclear cores. While the spatial resolution of Spitzer is poor, the great sensitivity of the data reveals the underlying galaxy merger remnant, and provides the first look at off-nuclear mid-infrared activity.
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© 2006 Astronomical Society of the Pacific.Attached Files
Published - Surace2006p9216Spitzer_Space_Telescope_New_Views_Of_The_Cosmos.pdf
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Surace2006p9216Spitzer_Space_Telescope_New_Views_Of_The_Cosmos.pdf
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- 24561
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- CaltechAUTHORS:20110727-090020355
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2011-07-27Created from EPrint's datestamp field
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2019-11-01Created from EPrint's last_modified field
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- Infrared Processing and Analysis Center (IPAC)
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- ASP Conference Series
- Series Volume or Issue Number
- 357