activity
20092022
most citedSpectral analysis of Kepler SPB and Beta Cep candidate stars

84 citations · 430 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2022★ 11 cited

The Gaia-ESO survey: A spectroscopic study of the young open cluster NGC 3293

T. Morel, A. Blazère, T. Semaan +24

We present a spectroscopic analysis of the GIRAFFE and UVES data collected by the Gaia-ESO survey for the young open cluster NGC 3293. Archive spectra from the same instruments obt…

astro-ph.SR2022★ 19 cited

The Gaia-ESO Survey: The analysis of the hot-star spectra

R. Blomme, S. Daflon, M. Gebran +44

The Gaia-ESO Survey (GES) is a large public spectroscopic survey that has collected, over a period of 6 years, spectra of ~ 10^5 stars. This survey provides not only the reduced sp…

astro-ph.SR2017★ 12 cited

Quiescent and active phases in Be stars: A WISE snapshot of young galactic open clusters

A. Granada, C. E. Jones, T. A. A. Sigut +4

Through the modelling of near-infrared photometry of star plus disk systems with the codes BEDISK/BERAY, we successfully describe the WISE photometric characteristics of Be stars i…

astro-ph.SR2017★ 28 cited

Chemical abundances of fast-rotating massive stars. I. Description of the methods and individual results

Constantin Cazorla, Thierry Morel, Yael Naze +4

Aims: Recent observations have challenged our understanding of rotational mixing in massive stars by revealing a population of fast-rotating objects with apparently normal surface…

astro-ph.EP2017★ 37 cited

Strong HI Lyman- variations from the 11 Gyr-old host star Kepler-444: a planetary origin ?

V. Bourrier, D. Ehrenreich, R. Allart +8

Kepler-444 provides a unique opportunity to probe the atmospheric composition and evolution of a compact system of exoplanets smaller than the Earth. Five planets transit this brig…

astro-ph.SR2017★ 13 cited

Critical study of the distribution of rotational velocities of Be stars; II: Differential rotation and some hidden effects interfering with the interpretation of the Vsin i parameter

J. Zorec, Y. Frémat, A. Domiciano de Souza +9

We assume that stars may undergo surface differential rotation to study its impact on the interpretation of and on the observed distribution of ratios of true ro…