Giving physical significance to the Hi-GAL * data: Determining the distance of cold dusty cores in the Milky Way

Astronomy and Astrophysics

Volumn 526, Issue 18, 2011, Pages

  Russeil, D ^a   Pestalozzi, M ^b   Mottram, J C ^c   Bontemps, S ^d,o   Anderson, L D ^a   Zavagno, A ^a   Beltran M T ^e   Bally, J ^g   Brand, J ^f   Brunt, C ^c   Cesaroni, R ^e   Joncas, G ^h   Marshall, D ⁱ   Martin, P ^j   Massi, F ^e   Molinari, S ^b   Moore, T ^k   Noriega Crespo, A ^l   Olmi, L ^e   Thompson, M A ^m   Wienen, M ⁿ   Wyrowski, F ⁿ   more..

^a AIX MARSEILLE UNIVERSITÉ   (France)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c UNIVERSITY OF EXETER   (United Kingdom)

^d LABORATOIRE D ASTROPHYSIQUE DE BORDEAUX   (France)

^e INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^f OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^g UNIVERSITY OF COLORADO   (United States)

^h UNIVERSITÉ LAVAL   (Canada)

ⁱ IRAP   (France)

^j UNIVERSITY OF TORONTO   (Canada)

^k LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^l CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^m UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

ⁿ MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^o OBSERVATOIRE DE BORDEAUX   (France)

more..

Author keywords

Galaxy: general; Galaxy: structure; H ii regions; infrared: general; Infrared: ISM; ISM: clouds

Indexed keywords

GALAXY: GENERAL; GALAXY: STRUCTURE; H II REGIONS; INFRARED: GENERAL; INFRARED: ISM; ISM : CLOUDS;

CLOUDS; INFRARED IMAGING; PHOTOMETRY; STARS; VELOCITY;

GALAXIES;

EID: 78651407516     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015852     Document Type: Article

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