Dust and Nebular Emission in Star Forming Galaxies

Details Dust and Nebular Emission in Star Forming Galaxies Dust and Nebular Emission in Star Forming Galaxies

2001-05-29

arxiv.org/abs/astro-ph/0105495v1

Astronomy and Astrophysics

Astrophysics

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

Scientific paper

Star forming galaxies exhibit a variety of physical conditions, from quiescent normal spirals to the most powerful dusty starbursts. In order to study these complex systems, we need a suitable tool to analyze the information coming from observations at all wavelengths. We present a new spectro-photometric model which considers in a consistent way starlight as reprocessed by gas and dust. We discuss preliminary results to interpret some observed properties of VLIRGs.

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