Dust and Nebular Emission in Star Forming Galaxies
Astrophysics
2016-01-27 v1
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.
Cite
@article{arxiv.astro-ph/0105495,
title = {Dust and Nebular Emission in Star Forming Galaxies},
author = {Pasquale Panuzzo and Alessandro Bressan and Gian Luigi Granato and Laura Silva and Luigi Danese},
journal= {arXiv preprint arXiv:astro-ph/0105495},
year = {2016}
}
Comments
8 pages, to be published in "The link between stars and cosmology", 26-30 March, 2001, Puerto Vallarta, Mexico, by Kluwer, eds. M. Chavez, A. Bressan, A. Buzzoni, and D. Mayya