First detection of NH3 (10 → 00) from a low mass cloud core. On the low ammonia abundance of the ρ Oph A core

Astronomy and Astrophysics

Volumn 402, Issue 3, 2003, Pages

  Liseau, R ^a   Larsson, B ^a   Brandeker, A ^a   Bergman, P ^b   Bernath, P ^c   Black, J H ^b   Booth, R ^b   Buat, V ^d   Curry, C ^c   Encrenaz, P ^e   Falgarone, E ^f   Feldman, P ^g   Fich, M ^c   Floren H ^a   Frisk, U ^h   Gerin, M ^f   Gregersen, E ⁱ   Harju, J ^j   Hasegawa, T ^k   Hjalmarson, A ^b   Johansson, L ^b   Kwok, S ^k   Lecacheux, A ^e   Liljestrom T ^l   Mattila, K ^j   Mitchell, G ^m   Nordh, L ⁿ   Olberg, M ^b   Olofsson, G ^a   Pagani, L ^e   Plume, R ^k   Ristorcelli, I ^o   Sandqvist, Aa ^a   Scheele F V ^h   Serra, G ^o   Tothill, N ^m   Volk, K ^k   Wilson, C ⁱ   more..

^a STOCKHOLM OBSERVATORY   (Sweden)

^b CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

^c UNIVERSITY OF WATERLOO   (Canada)

^d AIX MARSEILLE UNIVERSITÉ   (France)

^e OBSERVATOIRE DE PARIS   (France)

^f ECOLE NORMALE SUPÉRIEURE   (France)

^g NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^h SWEDISH SPACE CORPORATION   (Sweden)

ⁱ MCMASTER UNIVERSITY   (Canada)

^j UNIVERSITY OF HELSINKI   (Finland)

^k UNIVERSITY OF CALGARY   (Canada)

^l AALTO UNIVERSITY   (Finland)

^m SAINT MARY S UNIVERSITY   (Canada)

ⁿ Swedish National Space Board   (Sweden)

^o IRAP   (France)

more..

Author keywords

Clouds; ISM: individual objects: Oph A; Molecules; Stars: formation

Indexed keywords

AMMONIA; GALAXIES; GROUND STATE; MATHEMATICAL MODELS; METHANOL;

INDIVIDUAL OBJECTS; LOW MASS CLOUD CORE;

ASTROPHYSICS;

EID: 0037687318     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030343     Document Type: Letter

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