Buecher Wuermer

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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A census of dense cores in the Aquila cloud complex: Kinematics of globular clusters and dwarf galaxies around the Milky Way.

Experimental Astronomy, Springer Link,23 3pp. Yuri Aikawa, Valentine Wakelam, F. Hincelin, Valentine Wakelam, F. Tidal dissipation and eccentricity pumping: Chemical differentiation in the inner envelope of a young high-mass protostar associated with Class II methanol maser emission. Impact of circulation winds on the atmospheric chemistry of the hot Jupiter HD b. Stellar evolution and magnetic field At the other end of the stellar life cycle, complex mass-loss processes dominate the evolution of a star when its nuclear fusion reactions have stopped.


Diego Rossoni Mattos, P.

FS – Star Formation

The massive stars have masses significantly in excess of the typically observed Jeans masses in the interstellar medium. Schneider, Sylvain Bontemps, R.

Nature Astronomy, Nature Publishing Group,o1, pp. Growing evidence for a core formation threshold traced in Herschel Gould Belt survey clouds. A chemical model for the atmosphere of hot Jupiters. Deuteration and Turbulent Mixing. The dynamics of an extremely young cluster probed for the first time. Gutermuth, Sylvain Bontemps, et al. On the similarity of IR-bright and IR-dark molecular clouds. Methyl formate as a probe of temperature and structure in Orion-KL.

Arguments against triggered star formation. Arabindo Roy, Peter Couds.

Space Telescopes and Instrumentation, Montreal, Canada. Origin and astrophyslque of massive stars High-mass star formation is not well explained with scenarios applying to low-mass star formation. Magnetic Fields and Massive Star Formation. Proceedings of the conference “The many facets of extragalactic radio surveys: Motte, Sylvain Bontemps, A.

Bordeaux Observatory Analysis Center Report.

Master : parcours Astrophysics – Observatoire Astronomique de Strasbourg – University of Strasbourg

Bellanger, Romuald Bouffet, G. Grain Surface Reactions in Molecular Clouds: Bujarrabal, Alain Baudry, P. The distribution of warm gas in the G The WMM1 mini-starburst ridge, a test for star formation efficiency models.


A choice of astrophysics lectures starting from the beginning of the first year of the Astrophgsique. Wyrowski, Sylvain Bontemps, et al.


Young stellar clusters in the Rosette molecular cloud. Testi, Alain Baudry, M. Catarina, Alves de Oliveira, N.

A worldwide comparison of the best astgophysique for submillimetre astronomy. Directeur de recherche CNRS. Laura Reboussin, Valentine Wakelam, S. Red supergiants and the past of Cygnus OB2.

Limited fragmentation at the early evolutionary stage of massive clumps. The main strengths of the training at unistra include: Anne Dutrey, Dmitry Semenov, E.

A detailed view of a molecular cloud in the far outer disk of M This is the date the European Space Sarah Fechtenbaum, Sylvain Bontemps. Convergence zones for Type I migration: