Spatial variation of the cooling lines in the Orion Bar from Herschel/PACS

Astronomy and Astrophysics

Volumn 538, Issue , 2012, Pages

  Bernard Salas, J ^a   Habart, E ^a   Arab, H ^a   Abergel, A ^a   Dartois, E ^a   Martin, P ^b   Bontemps, S ^c   Joblin, C ^d   White, G J ^e,f   Bernard, J P ^d   Naylor, D ^g  

^a UNIVERSITÉ PARIS SUD   (France)

^b UNIVERSITY OF TORONTO   (Canada)

^c LABORATOIRE D ASTROPHYSIQUE DE BORDEAUX   (France)

^d IRAP   (France)

^e OPEN UNIVERSITY   (United Kingdom)

^f RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^g UNIVERSITY OF LETHBRIDGE   (Canada)

Author keywords

H II regions; infrared: general; ISM: individual objects: orion bar; ISM: lines and bands

Indexed keywords

DUST GRAINS; EMISSION LINES; EMISSION PROFILE; ENHANCED EMISSION; FAR-INFRARED; FINE STRUCTURES; H II REGIONS; HERSCHEL; INFRARED: GENERAL; ISM: INDIVIDUAL OBJECTS; ISM: LINES AND BANDS; LOCAL CONDITIONS; M-LINES; PHOTO-DISSOCIATION REGIONS; PHYSICAL PROCESS; RADIATIVE TRANSFER CODES; SMALL REGION; SPATIAL PROFILES; SPATIAL RESOLUTION; SPATIAL VARIATIONS; SPATIALLY RESOLVED;

IONIZATION; RADIATIVE TRANSFER; SPATIAL DISTRIBUTION; STARS;

COOLING;

EID: 84860139660     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118083     Document Type: Article

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