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Paper detail

Dust and Nebular Emission in Star Forming Galaxies

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.

preprint2001arXivOpen access
Pasquale PanuzzoAlessandro BressanGian Luigi GranatoLaura SilvaLuigi Danese
astro-ph
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Pasquale PanuzzoAlessandro BressanGian Luigi GranatoLaura SilvaLuigi Danese

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