Showing 1–20 of 21 results
/ Date/ Name
Feb 8, 2016Testing the asymptotic relation for period spacings from mixed modes of red giants observed with the Kepler missionNov 5, 2023MELCHIORS: The Mercator Library of High Resolution Stellar SpectroscopyNov 30, 2018Photometric detection of internal gravity waves in early-type stars observed by CoRoTOct 1, 2018Binary Asteroseismic Modelling: isochrone-cloud methodology and application to Kepler gravity-mode pulsatorsOct 18, 2016Preparing and correcting extracted BRITE observationsOct 18, 2016Understanding the photometric variability of ζ Ori AaAug 16, 2018Magnetic characterization and variability study of the magnetic SPB star o LupMar 13, 2019Period spacings of gravity modes in rapidly rotating magnetic stars I. Axisymmetric fossil field with poloidal and toroidal componentsJun 18, 2018Forward asteroseismic modeling of stars with a convective core from gravity-mode oscillations: parameter estimation and stellar model selectionJun 10, 2018On the sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence starsMay 2, 2018Forward seismic modelling of the pulsating magnetic B-type star HD 43317May 2, 2018Detection of magnetic fields in chemically peculiar stars observed with the K2 space missionFeb 2, 2018K2 photometry and HERMES spectroscopy of the blue supergiant rho Leo: rotational wind modulation and low-frequency wavesSep 8, 2017Magneto-asteroseismology of massive magnetic pulsatorsMay 4, 2018K2 space photometry reveals rotational modulation and stellar pulsations in chemically peculiar A and B starsNov 19, 2018On the photometric detection of Internal Gravity Waves in upper main-sequence stars I. Methodology and application to CoRoT targetsAug 7, 2019New $β$ Cep pulsators discovered with K2 space photometryApr 3, 2017Studying the photometric and spectroscopic variability of the magnetic hot supergiant $ζ$ Orionis AaMar 6, 2017The Most Massive Heartbeat: An In-depth Analysis of ι OrionisJul 11, 2015Kepler'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