Dust and nebular emission in star forming galaxies

被引：0
|
作者：
Panuzzo, P [1 ]
Bressan, A [1 ]
Granato, GL [1 ]
Silva, L [1 ]
Danese, L [1 ]
机构：
[1] SISSA, I-34014 Trieste, Italy
来源：
NEW QUESTS IN STELLAR ASTROPHYSICS: THE LINK BETWEEN STARS AND COSMOLOGY | 2002年 / 274卷
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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 able to analyze the information available 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 of its application to a sample of local VLIRGs.
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页码：171 / 174
页数：4
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