We review the application of the one-dimensional Mixing Length Theory (MLT) model of
convection in stellar interiors and low-mass stellar evolution. We summarize the history of …

The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical
property of the system, including the star-formation history, metal content, abundance …

Some compact objects observed in gravitational wave events have masses in the gap
between known neutron stars (NSs) and black holes (BHs). The nature of these mass gap …

The size of a planet is an observable property directly connected to the physics of its
formation and evolution. We used precise radius measurements from the California-Kepler …

Most structural and evolutionary properties of galaxies strongly rely on the stellar initial mass
function (IMF), namely the distribution of the stellar mass formed in each episode of star …

We have determined masses, stellar mass functions, and structural parameters of 112 Milky
Way globular clusters by fitting a large set of N-body simulations to their velocity dispersion …

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 …

BANYAN Σ is a new Bayesian algorithm to identify members of young stellar associations
within 150 pc of the Sun. It includes 27 young associations with ages in the range∼ 1–800 …

ABSTRACT I describe a method to transform a set of stellar evolution tracks onto a uniform
basis and then interpolate within that basis to construct stellar isochrones. This method …

The mass–luminosity relation for late-type stars has long been a critical tool for estimating
stellar masses. However, there is growing need for both a higher-precision relation and a …