Zobrazeno 1 - 10
of 39
pro vyhledávání: '"Alain Castets"'
Autor:
Alain Castets
En l'an 1902, l'amour fou entre le jeune dreyfusard Valentin et la rebelle Thi Maï lance une saga aux destins tragiques qui va traverser l'Indochine, dans un Vietnam fascinant, de la conquête coloniale à la défaite. Leurs deux filles métisses, S
Autor:
Emmanuel Caux, Alain Castets, Berengere Parise, Bertrand Lefloch, Cecilia Ceccarelli, Alexander G. G. M. Tielens, Sébastien Maret
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 453, pp.949
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 453, pp.949. ⟨10.1051/0004-6361:20054476⟩
HAL
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 453, pp.949
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 453, pp.949. ⟨10.1051/0004-6361:20054476⟩
HAL
Context : Despite the low cosmic abundance of deuterium (D/H ~ 1e-5), large degrees of deuterium fractionation in molecules are observed in star forming regions with enhancements that can reach 13 orders of magnitude, which current models have diffic
Autor:
Alexandre Faure, D. R. Flower, Emmanuel Caux, Alexander G. G. M. Tielens, Bertrand Lefloch, Sébastien Maret, Cecilia Ceccarelli, Alain Castets
Publikováno v:
Astronomy & Astrophysics. 442:527-538
We present observations of methanol lines in a sample of Class 0 low mass protostars. Using a 1-D radiative transfer model, we derive the abundances in the envelopes. In two sources of the sample, the observations can only be reproduced by the model
Publikováno v:
Astronomy & Astrophysics. 427:895-899
The HH 222 streamers in Orion and their associated non-thermal radio jet form a unique object, whose nature remains enigmatic. We have carried out a set of detailed millimeter observations around the non-thermal radio source in several transitions of
Autor:
Alain Castets, D. Russeil
Publikováno v:
Astronomy & Astrophysics. 417:107-114
We present 12 CO(1-0), 12 CO(2-1) and/or 13 CO(1-0) observations, obtained with the 15 m SEST telescope, in the direction of 252 southern HII regions located within 2 ◦ of the galactic plane and in the interval 280 ◦ < l < 355 ◦ . The data pres
Autor:
Alain Castets, Lars-Åke Nyman, M.J. McCaughrean, J. Knude, S. Heathcote, M. Andersen, Bo Reipurth
Publikováno v:
Astronomy & Astrophysics. 414:969-978
We present millimetre, optical, and near-infrared observations of M 16 in the vicinity of the Herbig-Haro ob- ject HH 216. The line profiles of the CO (J = 2−1) spectra are broad and consist of both emission originating from four warm molecular cor
Autor:
Alain Castets, David Teyssier, Cecilia Ceccarelli, Berengere Parise, Emmanuel Caux, Valentine Wakelam, Stéphanie Cazaux, A. G. G. M. Tielens
Publikováno v:
Astrophysical Journal, 593(1), L51-L55. IOP PUBLISHING LTD
While warm dense gas is prevalent around low-mass protostars, the presence of complex saturated molecules-the chemical inventory characteristic of hot cores-has remained elusive in such environments. Here we report the results of an IRAM 30 m study o
Autor:
Laurent Loinard, Emmanuel Dartois, Jean-Jacques Benayoun, Emmanuel Caux, C. Ceccarelli, Ch Vastel, Bertrand Lefloch, Alexander G. G. M. Tielens, Alain Castets
Publikováno v:
Planetary and Space Science. 50:1205-1213
We present the results of a search for the doubly deuterated form of formaldehyde (D2CO) in a large sample of objects associated to star-formation. D2CO was detected in nearly 20 low-mass protostars, a success rate of 100%, with [D2CO]/[H2CO] abundan
Autor:
Laurent Pagani, Emmanuel Caux, Juan R. Pardo, Sébastien Maret, Cecilia Ceccarelli, Alain Castets
Publikováno v:
Astronomy & Astrophysics. 383:L9-L13
We present ISO-LWS observations at high spectral resolution ($R \sim 10^{4}$) towards a cold molecular cloud in the line of sight of W49. The HD ground state transition at 112 μ m is detected, showing the first observation of this line in absorption
Publikováno v:
Astronomy & Astrophysics. 375:40-53
Using the IRAM 30 m and SEST 15 m telescopes we mapped an area covering 300 00 220 00 around IRAS 16293 2422 in the N2H + J =1 ! 0, H2CO J =3 1;3 ! 21;2 ,S iOJ =2 ! 1 J =3 ! 2a ndJ =5 ! 4 molecular transitions. Five positions were also observed in th