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

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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…

astro-ph20073 cited

Search for pulsation among suspected A-type binaries and the new multiperiodic Delta Scuti star HD217860

Yves Fremat, P. Lampens, P. Van Cauteren +9

We have explored a sample of suspected A-type binaries in a systematic way, both spectroscopically and photometrically. Due to their location in the H-R diagram, indications of pul…

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…

astro-ph20069 cited

Discovery of magnetic fields in three He variable Bp stars with He and Si spots

M. Briquet, S. Hubrig, M. Schoeller +1

It is essential for the understanding of stellar structure models of high mass stars to explain why constant stars, non-pulsating chemically peculiar hot Bp stars and pulsating sta…