L183 (L134N) Revisited II. The dust content

Astronomy and Astrophysics

Volumn 417, Issue 2, 2004, Pages 605-613

  Pagani, L ^a   Bacmann, A ^b   Motte, F ^c   Cambresy L ^d   Fich, M ^e   Lagache, G ^f   Miville Deschenes M A ^f,g   Pardo, J R ^h   Apponi, A J ⁱ  

^a OBSERVATOIRE DE PARIS   (France)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c DIF   (France)

^d OBSERVATOIRE DE STRASBOURG   (France)

^e UNIVERSITY OF WATERLOO   (Canada)

^f UNIVERSITÉ PARIS SUD   (France)

^g UNIVERSITY OF TORONTO   (Canada)

^h INSTITUTO DE ESTRUCTURA DE LA MATERIA   (Spain)

ⁱ UNIVERSITY OF ARIZONA   (United States)

Author keywords

ISM: abundances; ISM: dust, extinction; ISM: individual: L134N; ISM: individual: L183; ISM: molecules; ISM: structure

Indexed keywords

GAUSSIAN NOISE (ELECTRONIC); INFRARED RADIATION; MILLIMETER WAVES; MOLECULAR DYNAMICS; NUMERICAL ANALYSIS; OPACITY; PHOTOMETRY; RADIO TELESCOPES; SIGNAL TO NOISE RATIO;

EXTINCTION; ISM:ABUNDANCES; ISM:DUST; ISM:INDIVIDUAL:L134N; ISM:INDIVIDUAL:L183; ISM:MOLECULES; ISM:STRUCTURE;

GALAXIES;

EID: 1842789565     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034087     Document Type: Article

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