Showing 1–20 of 42 results
/ Date/ Name
Mar 11, 2019Mixing by overshooting and rotation in intermediate mass starsApr 7, 2022Formation of black holes in the pair-instability mass gap: evolution of a post-collision starNov 27, 2023Stellar Black Holes and Compact Stellar RemnantsOct 5, 2020Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up and $^{12}$C($α$, $γ$)$^{16}$O rate on the pair-instability black hole mass gapJul 1, 2019On the photometric signature of fast rotatorsSep 4, 2019Multiple stellar populations in NGC 1866. New clues from Cepheids and Colour-Magnitude DiagramMar 27, 2023Massive binary black holes from Population II and III starsNov 14, 2018Mode Classification in Fast-Rotating Stars using a Convolutional Neural Network: Model-Based Regular Patterns in $δ$ Scuti StarsNov 5, 2021A Fresh Look at AGB stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial-Final Mass RelationApr 7, 2022Formation of black holes in the pair-instability mass gap: Hydrodynamical simulations of a head-on massive star collisionSep 23, 2023Dissecting the Gaia HR diagram II. The vertical structure of the star formation history across the Solar CylinderNov 21, 2022Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVNAug 29, 2024The cosmic rate of Pair-Instability SupernovaeFeb 19, 2025A new prescription for the spectral properties of population III stellar populationsJun 25, 2024Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channelsNov 30, 2023A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst ProgenitorsMar 27, 2023Binary black hole mergers from Population III stars: uncertainties from star formation and binary star propertiesMay 13, 2020The Predicted Properties of Helium-Enriched Globular Cluster Progenitors at High RedshiftJan 8, 2025Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populationsApr 2, 2025Strikingly high fraction of fast rotators in Magellanic Cloud star clusters