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UV upturn of elliptical galaxies

Abstract:
We investigate the UV upturn phenomenon of elliptical galaxies by applying the binary model of hot subdwarfs of Han et al. (2002, 2003). Preliminary results show that the model provides a natural explanation for the UV upturn phenomenon and that the model could be used to detect low level recent star formation.
Publication status:
Published

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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
Role:
Author
Volume:
15
Issue:
1
Pages:
17-24
Publication date:
2006-01-01
ISSN:
1392-0049
URN:
uuid:fd4d23aa-e3af-4db5-a97a-21fe3369f0b4
Source identifiers:
29422
Local pid:
pubs:29422

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