A high-resolution study of the H I-H2 transition across the perseus molecular cloud

Astrophysical Journal

Volumn 748, Issue 2, 2012, Pages

  Lee, Min Young ^a   Stanimirović, Snežana ^a   Douglas, Kevin A ^b   Knee, Lewis B G ^c,d,e   Di Francesco, James ^d   Gibson, Steven J ^f   Begum, Ayesha ^a   Grcevich, Jana ^g   Heiles, Carl ^h   Korpela, Eric J ⁱ   Leroy, Adam K ^e   Peek, J E G ^g   Pingel, Nickolas M ^a   Putman, Mary E ^g   Saul, Destry ^g  

^a UNIVERSITY OF WISCONSIN MADISON   (United States)

^b NAIC   (Puerto Rico)

^c JOINT ALMA OBSERVATORY   (Chile)

^d NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^e NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^f WESTERN KENTUCKY UNIVERSITY   (United States)

^g Columbia University ^*  (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

dust, extinction; infrared: ISM; ISM: individual objects (Perseus); ISM: molecules; radio lines: ISM

Indexed keywords

EID: 84863356265     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/748/2/75     Document Type: Article

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