Showing 1–20 of 21 results
/ Date/ Name
Mar 27, 2026Formation and Evolution of [Wolf-Rayet] Planetary Nebulae through a Late Thermal PulseDec 4, 2025Local mixing length theory with compositional effects:\ First application to asymptotic giant branch evolutionMar 30, 2025The $i$-processes nucleosynthesis during the formation of He-rich hot-subdwarf starsFeb 28, 2023Uncertainties in the 12C+12C reaction rate and their impact on the composition of ultra-massive WDsFeb 1, 2022Chemistry and physical properties of the born-again planetary nebula HuBi 1Aug 10, 2021The importance of thermal torques on the migration of planets growing by pebble accretionJun 25, 2020An in-depth reanalysis of the alleged type Ia supernova progenitor Henize 2-428May 20, 2020Catalogue of central stars of planetary nebulae: Expanded editionMay 16, 2019Hot UV-bright stars of galactic globular clustersSep 27, 2016Post-AGB evolution much faster than previously thoughtMay 14, 2010New chemical profiles for the asteroseismology of ZZ Ceti starsJun 12, 2009On the possible existence of short-period g-mode instabilities powered by nuclear burning shells in post-AGB H-deficient (PG1159-type) starsJan 13, 2009On the formation of hot DQ white dwarfsOct 16, 2008Revisiting the theoretical DBV (V777 Her) instability strip: the MLT theory of convectionAug 26, 2008Modeling He-rich subdwarfs through the hot-flasher ScenarioDec 5, 2007Asteroseismological measurements on PG 1159-035, the prototype of the GW Vir variable starsSep 3, 2007Asteroseismological constraints on the coolest GW Vir variable star (PG 1159-type)PG 0122+200Oct 13, 2006Asteroseismological constraints on the pulsating planetary nebula nucleus (PG1159-type) RX J2117.1+3412Jul 3, 2006New nonadiabatic pulsation computations on full PG1159 evolutionary models: the theoretical GW Vir instability strip revisitedMar 31, 2006Full evolutionary models for PG1159 stars. Implications for the helium-rich O(He) stars