UV upturn of elliptical galaxies
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 sta...
Auteurs principaux: | Han, Z, Podsiadlowski, P, Lynas-Gray, A |
---|---|
Format: | Conference item |
Publié: |
2006
|
Documents similaires
-
A Binary Model for the UV-upturn of Elliptical Galaxies
par: Han, Z, et autres
Publié: (2007) -
A binary model for the UV-upturn of elliptical galaxies (MNRAS version)
par: Han, Z, et autres
Publié: (2007) -
The formation of hot subdwarf stars and its implications for the UV-upturn phenomenon of elliptical galaxies
par: Han, Z, et autres
Publié: (2010) -
Binary Stars as the Source of the Far-UV Excess in Elliptical Galaxies
par: Han, Z, et autres
Publié: (2007) -
Hot Subdwarfs in Binaries as the Source of the Far-UV Excess in
Elliptical Galaxies
par: Podsiadlowski, P, et autres
Publié: (2008)