287 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR12 papers
- University of LiègeBE11 papers
- Sorbonne UniversitéFR6 papers
- Institut de Recherche pour le DéveloppementFR5 papers
- Institute for Cross-Disciplinary Physics and Complex SystemsES5 papers
- Laboratoire de Physique de l'Ecole Normale SupérieureFR5 papers
- Laboratory for Ocean Physics and Satellite Remote SensingFR5 papers
- Consejo Superior de Investigaciones CientíficasES4 papers
- École Normale Supérieure - PSLFR4 papers
- IfremerFR4 papers
- Service Hydrographique et Océanographique de la MarineFR4 papers
- Universitat de les Illes BalearsES4 papers
5 papers · 1 filter
The Multiwavelength Picture of Star Formation in the Very Young Open Cluster NGC6383
Gregor Rauw, Michaël De Becker
We review the properties of the very young (2 Myr) open cluster NGC6383. The cluster is dominated by the massive binary HD159176 (O7V + O7V). The distance to NGC6383 is consistentl…
The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X
M. De Becker, G. Rauw, J. M. Pittard +4
An increasing number of early-type (O and Wolf-Rayet) colliding wind binaries (CWBs) is known to accelerate particles up to relativistic energies. In this context, non-thermal emis…
DECPHOT: an optimal deconvolution-based photometric reduction method
M. Gillon, P. Magain, V. Chantry +5
A high accuracy photometric reduction method is needed to take full advantage of the potential of the transit method for the detection and characterization of exoplanets, especiall…
Spectroscopy of Massive Stars
Yael Naze
Although rare, massive stars, being the main sources of ionizing radiation, chemical enrichment and mechanical energy in the Galaxy, are the most important objects of the stellar p…
NGC 6231: X-ray properties of the early-type star population
H. Sana, Y. Naze, E. Gosset +3
Based on a deep XMM-Newton observation of the young open cluster NGC 6231, we derive the main X-ray properties of its early-type star population. Among the 610 X-ray sources detect…