activity
20072023
most citedKepler observations of variability in B-type stars

142 citations · 428 across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2023

A search for magnetic Scuti stars in Kepler hybrid candidates

K. Thomson-Paressant, C. Neiner, P. Lampens +4

Numerous candidate hybrid stars of type Scuti - Doradus have been identified with the Kepler satellite. However, many of them lie outside the theoretically expected instabi…

astro-ph.SR2017★ 3 cited

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…

astro-ph.SR2016★ 21 cited

HD 41641: A classical Sct-type pulsator with chemical signatures of an Ap star

A. Escorza, K. Zwintz, A. Tkachenko +8

Among the known groups of pulsating stars, Sct stars are one of the least understood. Theoretical models do not predict the oscillation frequencies that observations reveal. Co…

astro-ph.SR2015★ 46 cited

Kepler's first view of O-star variability: K2 data of five O stars in Campaign 0 as a proof-of-concept for O-star asteroseismology

B. Buysschaert, C. Aerts, S. Bloemen +9

We present high-precision photometric light curves of five O-type stars observed with the refurbished {\it Kepler\/} satellite during its Campaign 0. For one of the stars, we also…

astro-ph.SR2014★ 2 cited

Asteroseismology and spectropolarimetry: opening new windows on the internal dynamics of massive stars

Stéphane Mathis, Coralie Neiner

In this article, we show how asteroseismology and spectropolarimetry allow to probe dynamical processes in massive star interiors. First, we give a summary of the state-of-the-art.…

astro-ph.SR2013★ 9 cited

Extensive study of HD 25558, a long-period double-lined binary with two SPB components

Á. Sódor, P. De Cat, D. J. Wright +33

We carried out an extensive observational study of the Slowly Pulsating B (SPB) star, HD 25558. The ~2000 spectra obtained at different observatories, the ground-based and MOST sat…