Stellar Evolution Challenge [PDF]
Abstract We report about the results of the Stellar Evolution Challenge, initiated at the Leiden Lorentz Center meeting “Fine-tuning stellar population models” (June, 2006).
Weiss, A. +4 more
openaire +2 more sources
Modeling of magneto-rotational stellar evolution [PDF]
While magnetic fields have long been considered significant for the evolution of magnetic non-degenerate stars and compact stars, it has become clear in recent years that, in fact, all stars are deeply affected by their effects. This is particularly true
Koh Takahashi, N. Langer
semanticscholar +1 more source
A Search for Stellar Siblings of the ∼200 Myr TOI-251 b Planetary System
Young planets (
Qinghui Sun +6 more
doaj +1 more source
Convective H–He interactions in massive population III stellar evolution models [PDF]
In Pop III stellar models convection-induced mixing between H- and He-rich burning layers can induce a burst of nuclear energy and thereby substantially alter the subsequent evolution and nucleosynthesis in the first massive stars.
O. Clarkson, F. Herwig
semanticscholar +1 more source
Multiple Stellar Evolution: a population synthesis algorithm to model the stellar, binary, and dynamical evolution of multiple-star systems [PDF]
In recent years, observations have shown that multiple-star systems such as hierarchical triple and quadruple-star systems are common, especially among massive stars.
A. Hamers +4 more
semanticscholar +1 more source
The fates of massive stars: exploring uncertainties in stellar evolution with metisse [PDF]
In the era of advanced electromagnetic and gravitational wave detectors, it has become increasingly important to effectively combine and study the impact of stellar evolution on binaries and dynamical systems of stars.
P. Agrawal +4 more
semanticscholar +1 more source
Intriguing Revelations from Lithium, Beryllium, and Boron
This is a report on some highlights of research on the rare light elements, lithium (Li), beryllium (Be), and boron (B), that were presented at my Henry Norris Russell Lecture in 2020 January.
Ann Merchant Boesgaard
doaj +1 more source
parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code [PDF]
We present the updated version of the code used to compute stellar evolutionary tracks in Padova. It is the result of a thorough revision of the major in put physics, together with the inclusion of the pre‐main sequence phase, not present in our previous
A. Bressan +6 more
semanticscholar +1 more source
Disentangling Stellar Age Estimates from Galactic Chemodynamical Evolution
Stellar ages are key for determining the formation history of the Milky Way, but are difficult to measure precisely. Furthermore, methods that use chemical abundances to infer ages may entangle the intrinsic evolution of stars with the chemodynamical ...
Jeff Shen +4 more
doaj +1 more source
First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time [PDF]
We present a new cosmological, magnetohydrodynamical simulation for galaxy formation: TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2 × 21603 dark matter particles and gas cells in a volume 50 comoving Mpc across.
A. Pillepich +10 more
semanticscholar +1 more source

