Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
LAM
LAM, France
Meudon, Observatoire, Meudon, Hauts-de-Seine, France
Paris, Observatoire, Meudon, France
Paris, Observatoire, Meudon, Hauts-de-Seine, France
Laboratoire d'Astronomie Spatiale, CNRS, BP 8, F-13376, Marseille Cedex 12, France
Observatoire de Paris-Meudon, France
Lab. d'Astrophysique de Marseille, CNRS, Univ. de Provence, France
Laboratoire d'Astronomie Spatiale, CNRS, BP 8, F-13376 Marseille Cedex 12, France
Laboratoire d'Astronomie Spatiale, Traverse du siphon, 13004 Marseille, France
Laboratoire d'Astronomie Spatiale, Traverse du siphon, F-13004 Marseille, France
Groupe Infrarouge Spatial, Observatoire de Meudon, 92190-Meudon, France
LAS, CNRS, Marseille, France
Laboratoire d'Astrophysique de Marseille, Traverse du siphon, F-13004 Marseille
Observatoire de Marseille, 2 place Le Verrier 13248 Marseille Cedex 4, France
Laboratoire d'Astrophysique de Marseille, CNRS & Université de Provence, BP 8, 13376, Marseille Cedex 12, France
Laboratoire d'Astrophysique de Marseille, CNRS & Univ. de Provence, BP 8, 13376 Marseille Cedex 12, France
Marseille, Observatoire, France
Haute-Provence, Observatoire, Saint-Michel-l'Observatoire, France
Laboratoire d'Astrophysique de Marseille, CNRS / INSU - Université de Provence, 13388 Marseille Cedex 13, France
Laboratoire d'Astrophysique de Marseille, CNRS & Université de Provence, BP 8, 13376 Marseille Cedex 12, France
Laboratoire d'Astrophysique de Marseille, CNRS & Université de Provence, BP 8, F-13376 Marseille Cedex 12, France
LAS, CNRS & Université de Provence, BP 8, F-13004 Marseille, FRANCE
Lab. d'Astrophysique de Marseille, France
17OH spin-rotation transition frequencies (Polehampton+, 2003)
A calculation of infrared spectra from dust in planetary nebulae.
A far-infrared molecular and atomic line survey of the Orion KL region
A Herschel study of the properties of starless cores in the Polaris Flare dark cloud region using PACS and SPIRE
A quantitative study of the 7.7 and 11.3 micron emission bands based on IRAS/LRS spectra
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