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Study of local infrared bright galaxies with HERSHCEL-PACS

Abstract:

Infrared bright galaxies (LIRGs and ULIRGs) represent the bulk of the cosmic infrared background and play a major role in the cosmic star formation and accretion histories. For this reason they have been subject of intensive studies at all wavelengths. However, being very dusty galaxies, one of the key wavelength range to understand their evolutionary stages and the physic involved, is the Mid-Far-Infrared and sub-millimeter window. Previous (IRAS and ISO) and current (SPITZER) infrared missi...

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Publisher copy:
10.1002/asna.200585002

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Journal:
Astronomische Nachrichten
Volume:
326
Issue:
7
Pages:
523-524
Publication date:
2005-01-01
DOI:
ISSN:
0004-6337
Source identifiers:
252235
Language:
English
Pubs id:
pubs:252235
UUID:
uuid:2297203e-a027-4be3-8748-260c90f9b860
Local pid:
pubs:252235
Deposit date:
2012-12-19

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