activity
20122016
most citedSimultaneous X-ray and optical spectroscopy of the Oef supergiant lambda Cep

47 citations · 158 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2016★ 26 cited

Observational signatures of past mass-exchange episodes in massive binaries: The case of HD 149 404

F. Raucq, G. Rauw, E. Gosset +4

Mass and momentum exchanges in close massive binaries play an important role in their evolution, and produce several observational signatures such as asynchronous rotation and alte…

astro-ph.SR2015★ 11 cited

Massive open star clusters using the VVV survey IV. WR 62-2, a new very massive star in the core of the VVV CL041 cluster

A. -N. Chené, S. Ramírez Alegría, J. Borissova +8

Context The ESO Public Survey VISTA Variables in the Vía Láctea (VVV) provides deep multi-epoch infrared observations for an unprecedented 562 sq. degrees of the Galactic bulge and…

astro-ph.SR2015★ 47 cited

Simultaneous X-ray and optical spectroscopy of the Oef supergiant lambda Cep

G. Rauw, A. Herve, Y. Naze +8

Probing the structures of stellar winds is of prime importance for the understanding of massive stars. Based on their optical spectral morphology and variability, the stars of the…

astro-ph.HE2013★ 15 cited

The Hot and Energetic Universe: Star formation and evolution

S. Sciortino, G. Rauw, M. Audard +16

Stars over a wide range of masses and evolutionary stages are nowadays known to emit X-rays. This X-ray emission is a unique probe of the most energetic phenomena occurring in the…

astro-ph.SR2013★ 41 cited

A detailed X-ray investigation of ζ Puppis III. A spectral analysis of the whole RGS spectrum

A. Hervé, G. Rauw, Y. Nazé

Context. Zeta Pup is the X-ray brightest O-type star of the sky. This object was regularly observed with the RGS instrument aboard XMM-Newton for calibration purposes, leading to a…

astro-ph.SR2012★ 18 cited

Global modelling of X-ray spectra produced in O-type star winds

A. Hervé, G. Rauw, Y. Nazé +1

High-resolution X-ray spectra of O-type stars revealed less wind absorption than expected from smooth winds with conventional mass-loss rates. Various solutions have been proposed,…