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20042008
most citedNon-thermal radio emission from single hot stars

20 citations · 20 across the 4 of their papers we have counts for

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astro-ph2008

The Gaia satellite: a tool for Emission Line Stars and Hot Stars

Christophe Martayan, Yves Fremat, Ronny Blomme +19

The Gaia satellite will be launched at the end of 2011. It will observe at least 1 billion stars, and among them several million emission line stars and hot stars. Gaia will provid…

astro-ph2007

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…

astro-ph2007

Three Dimensional Radiative Transfer in Winds of Massive Stars: Wind3D

A. Lobel, R. Blomme

We discuss the development of the new radiative transfer code Wind3D. It solves the non-LTE radiative transport problem in moving stellar atmosphere models in three geometric dimen…

astro-ph2006

Non-thermal radio emission from O-type stars. II. HD 167971

R. Blomme, M. De Becker, M. C. Runacres +2

HD 167971 is a triple system consisting of a 3.3-day eclipsing binary (O5-8 V + O5-8 V) and an O8 supergiant. It is also a well known non-thermal radio emitter. We observed the rad…

astro-ph200420 cited

Non-thermal radio emission from single hot stars

S. Van Loo, M. C. Runacres, R. Blomme

We present a theoretical model for the non-thermal radio emission from single hot stars, in terms of synchrotron radiation from electrons accelerated in wind-embedded shocks. The m…