Yearslong time series of high-precision brightness measurements have been assembled for
thousands of stars with telescopes operating in space. Such data have allowed astronomers …

▪ Abstract In this article we first review the main physical effects to be considered in the
building of evolutionary models of rotating stars on the Upper Main-Sequence (MS). The …

Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars in the
Metallicity Range −3 ≤ [Fe/H] ≤ 0 - IOPscience This site uses cookies. By continuing to use …

This is the first of a series of papers presenting the Modules for Experiments in Stellar
Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project, a new comprehensive …

During most of their life, stars fuse hydrogen into helium in their cores. The mixing of
chemical elements in the radiative envelope of stars with a convective core is able to …

We present a new comprehensive collection of stellar evolutionary tracks and isochrones for
rotating low-and intermediate-mass stars assembled with the updated version of PARSEC …

Context. After years of scientific progress, the origin of stellar binary black holes is still a
great mystery. Several formation channels for merging black holes have been proposed in …

We study the impact of mass-transfer physics on the observable properties of binary black
hole populations that formed through isolated binary evolution. We used the POSYDON …

Aims. Many topical astrophysical research areas, such as the properties of planet host stars,
the nature of the progenitors of different types of supernovae and gamma ray bursts, and the …

We present a dense grid of evolutionary tracks and isochrones of rotating massive main-
sequence stars. We provide three grids with different initial compositions tailored to compare …