The impact of thermally pulsing asymptotic giant branch stars on hierarchical galaxy formation models
The spectro-photometric properties of galaxies in galaxy formation models are obtained by combining the predicted history of star formation and mass accretion with the physics of stellar evolution through stellar population models. In the recent literature, significant differences have emerged regar...
Main Authors: | Tonini, C, Maraston, C, Devriendt, J, Thomas, D, Silk, J |
---|---|
Format: | Journal article |
Language: | English |
Published: |
2009
|
Similar Items
-
Hierarchical models of high redshift galaxies with thermally pulsing
asymptotic giant branch stars: comparison with observations
by: Tonini, C, et al.
Published: (2009) -
The impact of TP-AGB stars on hierarchical galaxy formation models
by: Tonini, C, et al.
Published: (2009) -
The hierarchical build-up of the Tully-Fisher relation
by: Tonini, C, et al.
Published: (2010) -
A POSSIBLE CRITERION FOR ENVELOPE EJECTION IN ASYMPTOTIC GIANT BRANCH OR 1ST GIANT BRANCH STARS
by: Han, Z, et al.
Published: (1994) -
Star formation losses due to tidal debris in `hierarchical' galaxy
formation
by: Roukema, B, et al.
Published: (2001)