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Formation des raies dans les vents des étoiles Ae/Be de Herbig
Herbig AejBe stars are pre-main sequence stars of intermediate masses (2-5 Mc) that exhibit strong signs of activity and stellar winds. The origin of these phenomenons... -
Numerical simulations of colliding winds in binary systems
The aim of this thesis is to understand the structure of colliding wind binaries composed of a massive star and a young pulsar, called gamma-ray binaries. They are...
