[HTML][HTML] The Initial-Final Mass Relation from Carbon Stars in Open Clusters
Recently, Marigo et al, identified a kink in the initial-final mass relation around initial masses
of M ini≈ 1.65− 2.10 M⊙, based on Gaia DR2 and EDR3 data for white dwarfs in open …
of M ini≈ 1.65− 2.10 M⊙, based on Gaia DR2 and EDR3 data for white dwarfs in open …
The White Dwarf Pareto: Tracing Mass Loss in Binary Systems
S Shahaf - arXiv preprint arXiv:2501.09586, 2025 - arxiv.org
The white dwarf mass distribution has been studied primarily at two extremes: objects that
presumably evolved as single stars and members of close binaries that likely underwent …
presumably evolved as single stars and members of close binaries that likely underwent …
Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC
Recent advancements in stellar evolution modeling offer unprecedented accuracy in
predicting the evolution and deaths of stars. We present new stellar evolutionary models …
predicting the evolution and deaths of stars. We present new stellar evolutionary models …
A combined study of thermohaline mixing and envelope overshooting with PARSEC: Calibration to NGC 6397 and M4
Thermohaline mixing is one of the main processes in low-mass red giant stars that affect the
transport of chemicals and, thus, the surface abundances along the evolution. The interplay …
transport of chemicals and, thus, the surface abundances along the evolution. The interplay …
The Initial-FinalMass Relation from Carbon Stars in Open Clusters
CA Abia Ladrón De Guevara, MI Domínguez Aguilera… - 2024 - digibug.ugr.es
Recently, Marigo et al, identified a kink in the initial-final mass relation around initial masses
of Mini≈ 1.65− 2.10 M⊙, based on Gaia DR2 and EDR3 data for white dwarfs in open …
of Mini≈ 1.65− 2.10 M⊙, based on Gaia DR2 and EDR3 data for white dwarfs in open …
Exoplanets, Low-mass Stars, and Binary Systems in the Era of Precision Radial Velocities and Astrometry
MR Giovinazzi - 2024 - search.proquest.com
Comprehensive investigations of gravitationally-bound systems based on data from ground-
and space-based missions offer the best opportunities to study a range of objects in our …
and space-based missions offer the best opportunities to study a range of objects in our …
The Initial-Final Mass Relation of White Dwarfs: Insights from PARSEC and COLIBRI TP-AGB models
F Addari - 2024 - tesidottorato.depositolegale.it
Abstract The Initial-Final Mass Relation (IFMR) plays a crucial role in understanding the
structure and evolution of stars, by linking the star's initial mass to the mass of its remnant. In …
structure and evolution of stars, by linking the star's initial mass to the mass of its remnant. In …