Globular cluster (GC) systems have now been studied in galaxies ranging from dwarfs to
giants and spanning the full Hubble sequence of morphological types. Imaging and …

After hydrogen and helium, oxygen, carbon, and nitrogen—hereinafter, the CNO elements—
are the most abundant species in the universe. They are observed in all kinds of …

Our understanding of the properties and demographics of exoplanets critically relies on our
ability to determine the fundamental properties of their host stars. The advent of Gaia and …

We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar
model and isochrone library for a solar-scaled heavy element distribution. The main input …

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 …

The ever-expanding depth and quality of photometric and spectroscopic observations of
stellar populations increase the need for theoretical models in regions of age-composition …

We substantially update the capabilities of the open source software package Modules for
Experiments in Stellar Astrophysics (MESA), and its one-dimensional stellar evolution …

The National Ignition Facility (NIF)[EI Moses, J. Phys.: Conf. Ser. 112, 012003 (2008);
https://lasers. llnl. gov/], completed in March 2009, is the highest energy laser ever …

We provide a set of stellar evolution and nucleosynthesis calculations that applies
established physics assumptions simultaneously to low-and intermediate-mass and massive …

Context. Rotational splittings are currently measured for several main sequence stars and a
large number of red giants with the space mission Kepler. This will provide stringent …