Evolution of dust in the Orion Bar with Herschel: I. Radiative transfer modelling

Astronomy and Astrophysics

Volumn 541, Issue , 2012, Pages

  Arab, H ^a   Abergel, A ^a   Habart, E ^a   Bernard Salas, J ^a   Ayasso, H ^a   Dassas, K ^a   Martin, P G ^b   White, G J ^c,d  

^a UNIVERSITÉ PARIS SUD   (France)

^b UNIVERSITY OF TORONTO   (Canada)

^c RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^d OPEN UNIVERSITY   (United Kingdom)

Author keywords

Dust, extinction; Infrared: ISM; ISM: individual objects: Orion Bar; Photon dominated region (PDR); Radiative transfer

Indexed keywords

DIFFUSE INTERSTELLAR MEDIUMS; DUST , EXTINCTION; DUST EMISSION; DUST GRAINS; HERSCHEL; INFRARED: ISM; INTERSTELLAR DUST; INTERSTELLAR MEDIUMS; IONIZATION FRONTS; ISM: INDIVIDUAL OBJECTS: ORION BARS; KEY ELEMENTS; LINE OF SIGHT; PHOTO-DISSOCIATION REGIONS; PHOTON-DOMINATED REGIONS; PHYSICAL CONDITIONS; RADIATIVE TRANSFER CODES; RADIATIVE TRANSFER MODEL; SPECTRAL EMISSIVITY; SPITZER; STAR FORMATIONS;

ASTRONOMY; COAGULATION; ELECTROMAGNETIC WAVE EMISSION; IONIZATION; LUMINANCE; PHOTODISSOCIATION; POLYCYCLIC AROMATIC HYDROCARBONS; RADIATIVE TRANSFER;

DUST;

EID: 84860156206     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118537     Document Type: Article

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