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A&A 406, L59-L62 (2003)
DOI: 10.1051/0004-6361:20030903
Letter
L183 (L134N) Revisited
I. The very cold core and the ridge
L. Pagani1, G. Lagache2, A. Bacmann3, F. Motte4, L. Cambrésy5, M. Fich6, D. Teyssier7, M.-A. Miville-Deschênes2, 8, J.-R. Pardo9, A. J. Apponi10 and B. Stepnik21 LERMA, UMR 8112 du CNRS, Observatoire de Paris, 61 Av. de l'Observatoire, 75014 Paris, France
2 IAS, Bât. 121, Université Paris-Sud, 91435 Orsay, France
3 ESO, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany
4 CEA, DSM, DAPNIA, Service d'Astrophysique, CE Saclay, 91191 Gif-sur-Yvette Cedex, France
5 Observatoire Astronomique de Strasbourg, UMR 7550, Université Louis Pasteur, 67000 Strasbourg, France
6 Physics Department, University of Waterloo, Waterloo, Ontario, N2L 3G1, Canada
7 SRON, PO Box 800, 9700 AV Groningen, The Netherlands
8 CITA, University of Toronto, 60 St. George Street, Toronto, Ontario, M5S 3H8, Canada
9 Instituto de Estructura de la Materia, Dpto de Física Molecular CSIC, Madrid, Spain
10 University of Arizona, Steward Observatory, 933 N. Cherry Ave., Tucson, AZ 85721, USA
(Received 24 March 2003 / Accepted 14 June 2003)
Abstract
We report new 1.2 mm continuum observations of the
L183
(=
L134N
) dark cloud with the MAMBO bolometer
array at IRAM. Combined with ISOCAM and ISOPHOT data at 7 and 200
m, this new observation is not compatible with the results found
by Ward-Thompson et al. (1994) with SCUBA and further
analysed by Lehtinen et al. (2003) using ISOPHOT
data. Only one bright core, with a northern elongation (the ridge) is
detected. We show that this core has an average temperature
K which is one of the coldest temperatures
reported so far.
Key words: ISM: dust, extinction -- ISM: structure -- ISM: individual: L134N -- ISM: individual: L183
Offprint request: L. Pagani, laurent.pagani@obspm.fr
SIMBAD Objects
© ESO 2003
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