activity
20022009
most citedDiscovery of magnetic fields in the beta Cephei star xi^1 CMa and in several Slowly Pulsating B stars

128 citations · 452 across the 11 of their papers we have counts for

collaborators

14 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-ph.SR20091 cited

Pulsations, chemical composition and multiplicity in main-sequence A- and F-type stars

S. Hekker, Y. Frémat, P. Lampens +1

The region in the HR-diagram where the main sequence intersects the classical instability strip hosts A- and F-type stars exhibiting a rich variety of physical phenomena, such as p…

astro-ph20083 cited

The seismology programme of CoRoT

E. Michel, A. Baglin, M. Auvergne +1

We introduce the main lines and specificities of the CoRoT Seismology Core Programme. The development and consolidation of this programme has been made in the framework of the CoRo…

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-ph200792 cited

A spectroscopic study of southern (candidate) gamma Doradus stars. II. Detailed abundance analysis and fundamental parameters

H. Bruntt, P. De Cat, C. Aerts

The gamma Doradus stars are a recent class of variable main sequence F-type stars located on the red edge of the Cepheid instability strip. They pulsate in gravity modes, and this…