Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-05-31
Mon.Not.Roy.Astron.Soc. 361 (2005) 725-742
Astronomy and Astrophysics
Astrophysics
19 pages and 14 figures. To appear in MNRAS. See http://www.bo.astro.it/~eps/home.html for more info on the models and data
Scientific paper
10.1111/j.1365-2966.2005.09204.x
We present here a new set of evolutionary population synthesis models for template galaxies along the Hubble morphological sequence. The models, that account for the individual evolution of the bulge, disk, and halo components, provide basic morphological features, along with bolometric luminosity and color evolution (including Johnson/Cousins "UBVRcIcJHK", Gunn "gri", and Washington "CMT1T2" photometric systems) between 1 and 15 Gyr. Luminosity contribution from residual gas is also evaluated, both in terms of nebular continuum and Balmer-line enhancement.
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