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26 April 2024
 
  » arxiv » astro-ph/0106128

 Article overview



Modelling the radio to X-ray SED of galaxies
Laura Silva ; Alessandro Bressan ; Gian Luigi Granato ; Pasquale Panuzzo ;
Date 7 Jun 2001
Subject astro-ph
AbstractWe 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.
Source arXiv, astro-ph/0106128
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