The Magnetism in Massive Stars (MiMeS) project represents the largest systematic survey of stellar magnetism ever undertaken. Based on a sample of over 550 Galactic B and O-type stars, the MiMeS project has derived the basic characteristics of magnetism in hot, massive stars. Herein we report preliminary results
We present the analysis performed on spectropolarimetric data of 97 O-type targets included in the f...
Massive stars are those stars with initial masses above about 8 times that of the sun, eventually le...
Published in MNRASInternational audienceWe present the analysis performed on spectropolarimetric dat...
peer reviewedThe MiMeS (Magnetism in Massive Stars) project is a large-scale, high-resolution, sensi...
The Magnetism in Massive Stars (MiMeS) Project is a consensus collaboration among many of the foremo...
We present the analysis performed on spectropolarimetric data of 97 O-type targets included in the f...
We present the analysis performed on spectropolarimetric data of 97 O-type targets included in the f...
Massive stars are those stars with initial masses above about 8 times that of the sun, eventually le...
Published in MNRASInternational audienceWe present the analysis performed on spectropolarimetric dat...
peer reviewedThe MiMeS (Magnetism in Massive Stars) project is a large-scale, high-resolution, sensi...
The Magnetism in Massive Stars (MiMeS) Project is a consensus collaboration among many of the foremo...
We present the analysis performed on spectropolarimetric data of 97 O-type targets included in the f...
We present the analysis performed on spectropolarimetric data of 97 O-type targets included in the f...
Massive stars are those stars with initial masses above about 8 times that of the sun, eventually le...
Published in MNRASInternational audienceWe present the analysis performed on spectropolarimetric dat...