M. Vučković

Magnetic spots on hot massive stars

Obliquities of exoplanet host stars

A new yield simulator for transiting planets and false positives: application to the Next Generation Transit Survey

An³He-DRIVEN INSTABILITY NEAR THE FULLY CONVECTIVE BOUNDARY

THE SURFACE NITROGEN ABUNDANCE OF A MASSIVE STAR IN RELATION TO ITS OSCILLATIONS, ROTATION, AND MAGNETIC FIELD

A Pan-STARRS 1 study of the relationship between wide binarity and planet occurrence in theKeplerfield

Presupernova Evolution of Massive Single and Binary Stars

ASTEROSEISMOLOGY OF THE NEARBY SN II PROGENITOR RIGEL. II. ϵ-MECHANISM TRIGGERING GRAVITY-MODE PULSATIONS?

MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS

Grids of stellar models with rotation : I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)

MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): PLANETS, OSCILLATIONS, ROTATION, AND MASSIVE STARS

CoRoT high-precision photometry of the B0.5 IV star HD 51756

Periodic mass-loss episodes due to an oscillation mode with variable amplitude in the hot supergiant HD 50064

Deviations from a uniform period spacing of gravity modes in a massive star

An asteroseismic study of the O9V star HD 46202 from CoRoT\n space-based photometry

Detection of frequency spacings in the young O-type binary HD 46149 \nfrom CoRoT photometry

K2-161b: a low-density super-Neptune on an eccentric orbit

AT LAST—A V777 HER PULSATOR IN THE KEPLER FIELD