Showing 21–40 of 80 results
/ Date/ Name
Jul 4, 2018Star-planet interactions. V. Dynamical and equilibrium tides in convective zonesMar 10, 2013Populations of rotating stars. - I. Models from 1.7 to 15 Msun at Z = 0.014, 0.006, and 0.002 with Ω/Ωcrit between 0 and 1Aug 13, 2013Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002Mar 23, 2012Grids of stellar models with rotation II. WR populations and supernovae/GRB progenitors at Z = 0.014Nov 25, 2025Precise mass and radius determination for two new and one known Neptune-sized planets around G Dwarf hostsApr 21, 2006Solar-like oscillations in the metal-poor subgiant nu Indi: constraining the mass and age using asteroseismologyJul 24, 2008A multi-site campaign to measure solar-like oscillations in Procyon. I. Observations, Data Reduction and Slow VariationsMay 3, 2021Standard solar models: a perspective from updated solar neutrino fluxes and the gravity-mode period spacingDec 8, 2021Asteroseismology of $β$ Cephei stars: The stellar inferences tested in hare and hound exercisesSep 8, 2014Table of Contents of: "Asteroseismology of Stellar Populations in the Milky Way"Sep 8, 2014Effects of rotation on stellar evolution and asteroseismology of red giantsMar 24, 2017Massive star formation by accretion II. Rotation: how to circumvent the angular momentum barrier?Jun 7, 2017Star-planet interactions. IV. Possibility of detecting the orbit-shrinking of a planet around a red giantDec 20, 2023Impact of different approaches for computing rotating stellar models I. The solar metallicity caseOct 20, 2009Nucleosynthesis in Rotating massive stars and Abundances in the Early GalaxyNov 14, 2008Models for Pop I stars: implications for age determinationsJul 9, 2024Grids of stellar models with rotation VIII: Models from 1.7 to 500 $M_\odot$ at metallicity $Z = 10^{-5}$Dec 13, 2023Dynamical tides in binaries: Inconsistencies in the implementation of Zahn's prescriptionApr 9, 2025Helioseismic inference of the solar radiative opacitySep 17, 2025The impact of rotational mixing in intermediate-age star clusters with extended main-sequence turn-offs and extended red clumps