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A new model for the infrared emission of IRAS F10214+4724

Abstract:

We present a new model for the infrared emission of the high redshift hyperluminous infrared galaxy IRAS F10214+4724 which takes into account recent photometric data from Spitzer and Herschel that sample the peak of its spectral energy distribution. We first demonstrate that the combination of the AGN tapered disc and starburst models of Efstathiou and coworkers, while able to give an excellent fit to the average spectrum of type 2 AGN measured by Spitzer, fails to match the spectral energy d...

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Publisher copy:
10.1017/S1743921312009064

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Journal:
Proceedings of the International Astronomical Union More from this journal
Volume:
7
Issue:
S284
Pages:
205-209
Publication date:
2011-09-01
DOI:
EISSN:
1743-9221
ISSN:
1743-9213
Language:
English
Keywords:
Pubs id:
pubs:351051
UUID:
uuid:ce1c312b-00b5-4b83-bddb-5d6303554a03
Local pid:
pubs:351051
Source identifiers:
351051
Deposit date:
2013-11-16

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