The 9.7 and 18 μ m silicate absorption profiles towards diffuse and molecular cloud lines-of-sight

Astronomy and Astrophysics

Volumn 526, Issue 18, 2011, Pages

  Van Breemen, J M ^a   Min, M ^a,b   Chiar, J E ^c   Waters, L B F M ^a,d   Kemper, F ^e,f   Boogert, A C A ^g   Cami, J ^c,h   Decin, L ^a,i   Knez, C ^j   Sloan, G C ^k   Tielens, A G G M ^l  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b UTRECHT UNIVERSITY   (Netherlands)

^c SETI INSTITUTE   (United States)

^d SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^e UNIVERSITY OF MANCHESTER   (United Kingdom)

^f INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^g CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^h UNIVERSITY OF WESTERN ONTARIO   (Canada)

ⁱ UNIVERSITY OF LEUVEN   (Belgium)

^j Bldg 142   (United States)

^k Department of Obstetrics Gynecology   (United States)

^l LEIDEN UNIVERSITY   (Netherlands)

more..

Author keywords

dust, extinction; evolution; infrared: ISM; ISM: clouds; techniques: spectroscopic

Indexed keywords

DUST , EXTINCTION; EVOLUTION; INFRARED: ISM; ISM : CLOUDS; TECHNIQUES: SPECTROSCOPIC;

ABSORPTION; CLOUDS; DUST; GRAIN GROWTH; PROBES;

SILICATES;

EID: 78651381285     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811142     Document Type: Article

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