232 citations · 2.2k across the 58 of their papers we have counts for
57 papers
Combined asteroseismology, spectroscopy, and astrometry of the CoRoT B2V target HD 170580
C. Aerts, M. G. Pedersen, E. Vermeyen +9
Space asteroseismology reveals that stellar structure and evolution models of intermediate- and high-mass stars are in need of improvement in terms of angular momentum and chemical…
Magnetic characterization of the SPB/ Cep hybrid pulsator HD 43317
B. Buysschaert, C. Neiner, M. Briquet +1
Large-scale magnetic fields at the surface of massive stars do not only influence the outer-most layers of the star, but also have consequences for the deep interior, only observat…
Magnetic field geometry and chemical abundance distribution of the He-strong star CPD -57 3509
S. Hubrig, N. Przybilla, H. Korhonen +9
The magnetic field of CPD -57 3509 was recently detected in the framework of the BOB (B fields in OB stars) collaboration. We acquired low-resolution spectropolarimetric observatio…
Photometric and spectroscopic variability of the B5IIIe star HD 171219
L. Andrade, E. Janot-Pacheco, M. Emilio +11
We analyzed the star HD 171219, one of the relatively bright Be stars observed in the seismo field of the CoRoT satellite, in order to determine its physical and pulsation characte…
Detection of Solar-Like Oscillations, Observational Constraints, and Stellar Models for Cyg, the Brightest Star Observed by the {\it Kepler} Mission
J. A. Guzik, G. Houdek, W. J. Chaplin +52
Cygni is an F3 spectral-type main-sequence star with visual magnitude V=4.48. This star was the brightest star observed by the original Kepler spacecraft mission. Short-cadence…
Weak magnetic field, solid-envelope rotation, and wave-induced N-enrichment in the SPB star Cassiopeiae
M. Briquet, C. Neiner, P. Petit +3
Aims. The main-sequence B-type star Cassiopeiae is known as a N-rich star with a magnetic field discovered with the Musicos spectropolarimeter. We model the magnetic field of t…