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Dust and Nebular Emission in Star Forming Galaxies

Pasquale Panuzzo·Alessandro Bressan·Gian Luigi Granato·Laura Silva·Luigi Danese
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Abstract

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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Pasquale Panuzzo, Alessandro Bressan, Gian Luigi Granato, Laura Silva, Luigi Danese. 2001-05-29. Dust and Nebular Emission in Star Forming Galaxies. https://doi.org/10.1007/978-94-010-0393-3_35

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