Hints about the multiplicity of WR 133 based on multiepoch radio observations

Resolved astrometric orbits of ten O-type binaries

(2017) J.-B. Le Bouquin et al.   ASTRONOMY & ASTROPHYSICS

An investigation into the fraction of particle accelerators among colliding-wind binaries

(2017) M. De Becker et al.   ASTRONOMY & ASTROPHYSICS

Is the Stellar System WR 11 a Gamma-Ray Source?

(2016) Paula Benaglia   PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA

Radio emission from supernova remnants

(2015) Gloria Dubner et al.   ASTRONOMY AND ASTROPHYSICS REVIEW

Catalogue of particle-accelerating colliding-wind binaries

(2013) M. De Becker et al.   ASTRONOMY & ASTROPHYSICS

AN ACCURATE FLUX DENSITY SCALE FROM 1 TO 50 GHz

(2013) R. A. Perley et al.   ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

Evidence for a physically bound third component in HD 150136

(2012) L. Mahy et al.   ASTRONOMY & ASTROPHYSICS

Predictions for mass-loss rates and terminal wind velocities of massive O-type stars

(2011) L. E. Muijres et al.   ASTRONOMY & ASTROPHYSICS

Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae

(2011) Stephen P. Reynolds et al.   SPACE SCIENCE REVIEWS

Non-thermal radio emission from O-type stars

(2010) R. Blomme et al.   ASTRONOMY & ASTROPHYSICS

DISENTANGLING THE NATURE OF THE RADIO EMISSION IN WOLF-RAYET STARS

(2009) Gabriela Montes et al.   ASTROPHYSICAL JOURNAL