Multiple populations in star clusters
AP Milone, AF Marino - Universe, 2022 - mdpi.com
We review the multiple population (MP) phenomenon of globular clusters (GCs): ie, the
evidence that GCs typically host groups of stars with different elemental abundances and/or …
evidence that GCs typically host groups of stars with different elemental abundances and/or …
Models of very-low-mass stars, brown dwarfs and exoplanets
F Allard, D Homeier, B Freytag - … Transactions of the …, 2012 - royalsocietypublishing.org
Within the next few years, GAIA and several instruments aiming to image extrasolar planets
will be ready. In parallel, low-mass planets are being sought around red dwarfs, which offer …
will be ready. In parallel, low-mass planets are being sought around red dwarfs, which offer …
Mesa isochrones and stellar tracks (MIST). I. Solar-scaled models
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 …
Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project, a new comprehensive …
MESA Isochrones and Stellar Tracks (MIST) 0: methods for the construction of stellar isochrones
A Dotter - The Astrophysical Journal Supplement Series, 2016 - iopscience.iop.org
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 …
basis and then interpolate within that basis to construct stellar isochrones. This method …
Improving PARSEC models for very low mass stars
Many stellar models present difficulties in reproducing basic observational relations of very
low mass stars (VLMS), including the mass–radius relation and the optical colour …
low mass stars (VLMS), including the mass–radius relation and the optical colour …
Observing the atmospheres of known temperate Earth-sized planets with JWST
CV Morley, L Kreidberg, Z Rustamkulov… - The Astrophysical …, 2017 - iopscience.iop.org
Nine transiting Earth-sized planets have recently been discovered around nearby late-M
dwarfs, including the TRAPPIST-1 planets and two planets discovered by the MEarth survey …
dwarfs, including the TRAPPIST-1 planets and two planets discovered by the MEarth survey …
Galactic stellar and substellar initial mass function1
G Chabrier - Publications of the Astronomical Society of the …, 2003 - iopscience.iop.org
We review recent determinations of the present‐day mass function (PDMF) and initial mass
function (IMF) in various components of the Galaxy—disk, spheroid, young, and globular …
function (IMF) in various components of the Galaxy—disk, spheroid, young, and globular …
On the variation of the initial mass function
P Kroupa - Monthly Notices of the Royal Astronomical Society, 2001 - academic.oup.com
A universal initial mass function (IMF) is not intuitive, but so far no convincing evidence for a
variable IMF exists. The detection of systematic variations of the IMF with star-forming …
variable IMF exists. The detection of systematic variations of the IMF with star-forming …
Evolutionary models for solar metallicity low-mass stars: mass-magnitude relationships and color-magnitude diagrams
We present evolutionary models for low mass stars from 0.075 to 1$\msol $ for solar-type
metallicities [M/H]= 0 and-0.5. The calculations include the most recent interior physics and …
metallicities [M/H]= 0 and-0.5. The calculations include the most recent interior physics and …
Evolutionary models for very low-mass stars and brown dwarfs with dusty atmospheres
We present evolutionary calculations for very low-mass stars and brown dwarfs based on
synthetic spectra and nongray atmosphere models which include dust formation and …
synthetic spectra and nongray atmosphere models which include dust formation and …