Changes of dust opacity with density in the orion a molecular cloud

Astrophysical Journal

Volumn 763, Issue 1, 2013, Pages

  Roy, Arabindo ^a   Martin, Peter G ^a   Polychroni, Danae ^b   Bontemps, Sylvain ^c   Abergel, Alain ^d   André, Philippe ^e   Arzoumanian, Doris ^e   Di Francesco, James ^f   Hill, Tracey ^e   Konyves, Vera ^d,e   Nguyen Luong, Quang ^a   Pezzuto, Stefano ^g   Schneider, Nicola ^c,e   Testi, Leonardo ^h   White, Glenn ^i,j  

^a UNIVERSITY OF TORONTO   (Canada)

^b INAF   (Italy)

^c UNIVERSITÉ DE BORDEAUX   (France)

^d UNIVERSITÉ PARIS SUD   (France)

^e UNIVERSITÉ PARIS DIDEROT   (France)

^f NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^g INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^h EUROPEAN SOUTHERN OBSERVATORY   (Germany)

ⁱ OPEN UNIVERSITY   (United Kingdom)

^j STFC Rutherford Appleton Laboratory ^*  (United Kingdom)

more..

Author keywords

dust, extinction; evolution; infrared: ISM; ISM: general; ISM: structure; submillimeter: ISM

Indexed keywords

EID: 84872221401     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/763/1/55     Document Type: Article

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