Rotation and the associated mixing has recently been included in massive star evolutionary models in an attempt to reconcile theory with observation, e.g surface abundance anomalies, such as nitrogen enrichments. However, despite the apparent importance of rotation there have been few observational tests, specifically in regard to fast rotating stars. This thesis presents the analysis of the Magellanic Cloud B-type stars from the 'The VLT-FLAMES survey of massive stars'. Atmospheric paramaters and rotational velocities have been estimated for rv400 objects, with chemical compositions being derived for over half this sample. This represents the largest homogenous survey undertaken to date. Comparison of the rotational velocity distributions ...
Context. With growing evidence for the existence of very massive stars at subsolar metallicity, ther...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
Aims. We have previously analysed the spectra of 135 early B-type stars in the Large Magellanic Clou...
Aims. We have previously analysed the spectra of 135 early B-type stars in the Large Magellanic Clou...
Rotation has become an important element in evolutionary models of massive stars, specifically via t...
Context. Rotational mixing in massive stars is a widely applied concept, with far-reaching consequen...
Context. Rotational mixing in massive stars is a widely applied concept, with far-reaching consequen...
International audienceAims:We aim to provide the atmospheric parameters and rotational velocities fo...
International audienceAims:We aim to provide the atmospheric parameters and rotational velocities fo...
International audienceAims:We aim to provide the atmospheric parameters and rotational velocities fo...
Aims.We aim to provide the atmospheric parameters and rotational velocities for a large sample of O-...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
Context. With growing evidence for the existence of very massive stars at subsolar metallicity, ther...
Context. With growing evidence for the existence of very massive stars at subsolar metallicity, ther...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
Aims. We have previously analysed the spectra of 135 early B-type stars in the Large Magellanic Clou...
Aims. We have previously analysed the spectra of 135 early B-type stars in the Large Magellanic Clou...
Rotation has become an important element in evolutionary models of massive stars, specifically via t...
Context. Rotational mixing in massive stars is a widely applied concept, with far-reaching consequen...
Context. Rotational mixing in massive stars is a widely applied concept, with far-reaching consequen...
International audienceAims:We aim to provide the atmospheric parameters and rotational velocities fo...
International audienceAims:We aim to provide the atmospheric parameters and rotational velocities fo...
International audienceAims:We aim to provide the atmospheric parameters and rotational velocities fo...
Aims.We aim to provide the atmospheric parameters and rotational velocities for a large sample of O-...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
Context. With growing evidence for the existence of very massive stars at subsolar metallicity, ther...
Context. With growing evidence for the existence of very massive stars at subsolar metallicity, ther...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
International audienceContext. Massive star evolution remains only partly constrained. In particular...