Modelling the radio to X-ray SED of galaxies

Details Modelling the radio to X-ray SED of galaxies Modelling the radio to X-ray SED of galaxies

2001-06-07

arxiv.org/abs/astro-ph/0106128v1

Astronomy and Astrophysics

Astrophysics

4 pages, to be published in "The link between stars and cosmology", 26-30 March, 2001, Puerto Vallarta, Mexico, by Kluwer, eds

Scientific paper

We present our model to interpret the SED of galaxies. The model for the UV
to sub-mm SED is already well established (Silva et al 1998). We remind here
its main features and show some applications. Recently we have extended the
model to the radio range (Bressan et al 2001), and we have started to include
the X-ray emission from the stellar component.

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