Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
Scientist
AIME, SAp
DAPNIA / DSM / CEA Centre d'Etudes de Saclay
Service d'Astrophysique / DAPNIA / DSM / CEA Saclay, F-91191 Gif-sur-Yvette, France
Laboratoire AIM Saclay Paris, CEA, France
Onsala Space Observatory, 439 92 Onsala, Sweden
CEA, DSM, IRFU, Service d'Astrophysique, France
IRFU / SAp CEA / DSM, Laboratoire AIM CNRS - Université Paris Diderot, France
UNSW
AIM, Irfu
Service d'Astrophysique, DAPNIA / DSM / CEA Saclay, France
Service d'Astrophysique, DAPNIA / DSM / CEA Saclay, 91191 Gif-sur-Yvette, France
Onsala Space Observatory
CEA, Lab. AIM, CNRS, France
Onsala Space Observatory, S-439 92 Onsala, Sweden
Department of Astrophysics, School of Physics, University of New South Wales, Sydney 2052, Australia
Onsala Space Observatory, S-43992 Onsala, Sweden
Service d'Astrophysique, DAPNIA / DSM / CEA CE de Saclay, 91191 Gif-sur-Yvette, France; AIM, Unité Mixte de Recherche, CEA-CNRS-Université Paris VII, UMR 7158, CEA / Saclay, 91191 Gif sur Yvette, France
IRFU / SAp, Commissariat à l'énergie atomique, Saclay, France
Service d'Astrophysique, DAPNIA / DSM / CEA Saclay, 91191 Gif-sur-Yvette, France; AIM, UMR 7158, CEA-CNRS-Université Paris VII, CEA / Saclay, 91191 Gif sur Yvette, France
Laboratoire AIM, CEA / IRFU - CNRS / INSU - Université Paris Diderot, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
Department of Astrophysics and Optics, School of Physics, University of New South Wales, NSW 2052, Australia; Onsala Space Observatory, 439 92 Onsala, Sweden
Onsala Space Observatory, 439 92 Onsala, Sweden; Department of Astrophysics and Optics, School of Physics, University of New South Wales, NSW 2052, Australia
School of Physics, University of New South Wales, Sydney 2052, NSW, Australia; Onsala Space Observatory, 439 92 Onsala, Sweden
CEA / Saclay / DSM / DAPNIA / SAp-SIS, UMR CEA / CNRS / UP7 Lab. AIM, France
3D simulations of pillars formation around HII regions: the importance of shock curvature
4 GHz cryogenic low noise IF amplifiers for OSO imaging receiver.
6.7GHz methanol masers survey of low-mass YSO (Minier+, 2003)
A CH3CN and HCO+ survey towards southern methanol masers associated with star formation
A general catalogue of 6.7 GHz methanol masers. I: data
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