A post-iras interstellar dust model
Identifieur interne : 000089 ( France/Analysis ); précédent : 000088; suivant : 000090A post-iras interstellar dust model
Auteurs : Francois-Xavier Desert [États-Unis] ; Francois Boulanger [États-Unis] ; Michel Pérault [France]Source :
- Lecture Notes in Physics [ 0075-8450 ] ; 1988.
Abstract
Abstract: A composite interstellar dust model is built in order to understand the infrared colors of various astronomical objects including the low-density interstellar medium (HI, H2, and HII) in cirrus, reflection nebulae, and HII regions. Taking into account the various constraints on the different dust components, in particular coming from IRAS data, we show that a bimodal rather than continuous size distribution between small and big grains is the most favorable solution.
Url:
DOI: 10.1007/BFb0118798
Affiliations:
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ISTEX:C24DAEA3E085BD7080B448B84B8494810061E370Le document en format XML
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