Showing 1–20 of 47 results
/ Date/ Name
Jul 9, 2009Ledoux's convection criterion in evolution and asteroseismology of massive starsJul 30, 2012Seismic signature of envelope penetrative convection: the CoRoT star HD 52265Aug 31, 2020SPInS, a pipeline for massive stellar parameter inference: A public Python tool to age-date, weigh, size up stars, and moreJun 3, 2014Asteroseismology for "à la carte" stellar age-dating and weighing: Age and mass of the CoRoT exoplanet host HD 52265Jan 7, 2008CoRoT/ESTA-TASK 1 and TASK 3 comparison of the internal structure and seismic properties of representative stellar models: Comparisons between the ASTEC, CESAM, CLES, GARSTEC and STAROX codesMay 29, 2001The Helium content and age of the Hyades: Constraints from five binary systems and Hipparcos parallaxesMar 23, 2000Stellar Structure and Evolution: Deductions from HipparcosOct 20, 2014How accurate are stellar ages based on stellar models? II. The impact of asteroseismologyApr 19, 2001Comparative seismology of pre- and main sequence stars in the instability stripJan 14, 2008CESAM: a free code for stellar evolution calculationsAug 29, 2008Reference grids of stellar models and oscillation frequencies: Data from the CESAM stellar evolution code and ADIPLS oscillation programmeNov 18, 2008Stellar ages from asteroseismologyAug 31, 2011Ages of Exoplanet Host-Stars from Asteroseismology : HD 17156, a Case StudyDec 11, 2013Impact of asteroseismology on improving stellar ages determinationOct 20, 2014How accurate are stellar ages based on stellar models ? I. The impact of stellar models uncertaintiesJun 2, 2023The surface composition of six newly discovered chemically peculiar stars. Comparison to the HgMn stars $μ$ Lep and $β$ Scl and the superficially normal B star $ν$ CapJun 14, 2023The unexpected optical and ultraviolet variability of the standard star $α$ Sex (HD 87887)Dec 1, 2016Standing on the shoulders of Dwarfs: the $Kepler$ asteroseismic LEGACY sample I - oscillation mode parametersJan 9, 2001Oscillation power as a test of stellar turbulence : Scanning the HR diagramApr 9, 2025Helioseismic inference of the solar radiative opacity