activity
20062009
most citedAn asteroseismic study of the beta Cephei star theta Ophiuchi: constraints on global stellar parameters and core overshooting

145 citations · 401 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR200964 cited

New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars

S. Hubrig, M. Briquet, P. De Cat +3

We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowl…

astro-ph.SR2009

New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars

S. Hubrig, M. Briquet, P. De Cat +3

We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowl…

astro-ph200828 cited

New insights into the nature of the peculiar star theta Carinae

S. Hubrig, M. Briquet, T. Morel +3

We acquired high resolution spectroscopic and low resolution spectropolarimetric observations to achieve the following goals: a) to improve the orbital parameters to allow a more i…

astro-ph2008123 cited

Nitrogen enrichment, boron depletion and magnetic fields in slowly-rotating B-type dwarfs

T. Morel, S. Hubrig, M. Briquet

Evolutionary models for massive stars, accounting for rotational mixing effects, do not predict any core-processed material at the surface of B dwarfs with low rotational velocitie…

astro-ph2007145 cited

An asteroseismic study of the beta Cephei star theta Ophiuchi: constraints on global stellar parameters and core overshooting

M. Briquet, T. Morel, A. Thoul +5

We present a seismic study of the beta Cephei star theta Ophiuchi. Our analysis is based on the observation of one radial mode, one rotationally split l = 1 triplet and three compo…

astro-ph200732 cited

On the co-existence of chemically peculiar Bp stars, slowly pulsating B stars and constant B stars in the same part of the H-R diagram

M. Briquet, S. Hubrig, P. De Cat +3

Aims. In order to better model massive B-type stars, we need to understand the physical processes taking place in slowly pulsating B (SPB) stars, chemically peculiar Bp stars, and…