Comparison of Far-IR and CO emission from nearby molecular clouds
Identifieur interne : 000914 ( Main/Exploration ); précédent : 000913; suivant : 000915Comparison of Far-IR and CO emission from nearby molecular clouds
Auteurs : F. Boulanger [États-Unis]Source :
- Lecture Notes in Physics [ 0075-8450 ] ; 1988.
Abstract
Abstract: We discuss the respective contributions of the interstellar radiation field and embedded stars to the heating of dust in molecular clouds, and present results of a comparison between far-IR and CO emission from nearby molecular clouds.
Url:
DOI: 10.1007/3-540-50438-9_238
Affiliations:
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Le document en format XML
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<front><div type="abstract" xml:lang="en">Abstract: We discuss the respective contributions of the interstellar radiation field and embedded stars to the heating of dust in molecular clouds, and present results of a comparison between far-IR and CO emission from nearby molecular clouds.</div>
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