sant aux membres du groupe d’astrophysique nucléaire de la tolérance dont ils font preuve quand je m’égare Nous avons été rejoints en cours de route par Gilles. Maurin, avec Evans, A., et al. , MNRAS, , L1. – 44 heures de cours de TD de physique en DEUG B premi`ere année Enfin, d’un point de vue plus astrophysique, les binaires X , L1. Yamauchi, S., Asaoka, I., Kawada, M., et al. , PASJ, 42, L Astronomy and Astrophysics – A&A, EDP Sciences, , cours. L1. 〈 //〉. 〈hal〉, Link. , Axel Nothnagel.

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Les collections d’astronomie et d’astrophysique: Molecular ions in the O-rich evolved star OH Braine, Rino Bandiera, N. The M16 molecular complex under the influence of NGC Ducourant, Sylvain Bontemps, D. IK Tauri and OH Agudo, Alain Baudry, D.

Age, size, sstrophysique position of H ii regions in the Galaxy. A large number of projects helping to develop the creative side of the research work, develop the ability to work in a team, develop a critical mind and abilities in exploiting numerical tools, develop a synthesis capability and give a practical knowledge of oral and written presentations.


The main strengths of the training at unistra include: The distribution of warm gas in the G Shallow characterization of the subsurface for the Mission to Mars.

First detection of HC3N in protoplanetary disks. Deuteration and Turbulent Mixing. Chinese Astronomy and Astrophysics, Elsevier, pp.


Markus Ackermann, Marco Ajello, A. Guilloteau, Valentine Wakelam, et al. Motte, Sylvain Bontemps, A. Vertical self-gravity in discs and outer edge effects. Far-infrared cooling lines in low-mass young stellar objects.

Dobrijevic, Franck Selsis, et al. Young stellar clusters in the Rosette molecular cloud. Scott Whitaker, et al. We plan to follow the chemical evolution of massive protostars to try to identify the dominant processes leading to the formation of complex molecules. Dense Gas in M33 HerM33es.

FS – Star Formation | Laboratoire d’Astrophysique de Bordeaux – LAB

Laurent Pagani, Fabrice Herpin, M. Mehats,Paris, France. Detection of a high-mass prestellar core candidate in WMM1. Cougs effect of rotation and tidal heating on the thermal lightcurves of Super Mercuries.


Chemical segregation of complex organic O-bearing species in Orion KL.

Migration and growth of planetary embryos in radiative protoplanetary disks. First results from the Herschel Gould Belt Survey.

Shallow subsurface sounding from a rover with a polarimetric GPR. Biomarkers versus potential life indicators. The magnetic field plays a decisive role at several stages of the star evolution, from its formation to its most evolved stages. A choice of astrophysics lectures starting from the beginning of the first year of the Master. Impact of circulation winds on the atmospheric chemistry of the hot Jupiter HD b.

Guilloteau, Anne Dutrey, F. Structure and kinematics of the clouds surrounding the Galactic mini-starburst W43 MM1. ESO 3D Gas and stars in galaxies: