Star Clusters Near and Far: Tracing Star Formation Across Cosmic Time
Star clusters are fundamental units of stellar feedback and unique tracers of their host
galactic properties. In this review, we will first focus on their constituents, ie detailed insight …
galactic properties. In this review, we will first focus on their constituents, ie detailed insight …
The role of magnetic fields in setting the star formation rate and the initial mass function
MR Krumholz, C Federrath - Frontiers in Astronomy and Space …, 2019 - frontiersin.org
Star-forming gas clouds are strongly magnetized, and their ionization fractions are high
enough to place them close to the regime of ideal magnetohydrodyamics on all but the …
enough to place them close to the regime of ideal magnetohydrodyamics on all but the …
Stars, gas, and dark matter in the solar neighborhood
CF McKee, A Parravano… - The Astrophysical …, 2015 - iopscience.iop.org
STARS, GAS, AND DARK MATTER IN THE SOLAR NEIGHBORHOOD - IOPscience This
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
Observational evidence of dynamic star formation rate in milky way giant molecular clouds
EJ Lee, MA Miville-Deschênes… - The Astrophysical …, 2016 - iopscience.iop.org
Star formation on galactic scales is known to be a slow process, but whether it is slow on
smaller scales is uncertain. We cross-correlate 5469 giant molecular clouds (GMCs) from a …
smaller scales is uncertain. We cross-correlate 5469 giant molecular clouds (GMCs) from a …
STARFORGE: the effects of protostellar outflows on the IMF
The initial mass function (IMF) of stars is a key quantity affecting almost every field of
astrophysics, yet it remains unclear what physical mechanisms determine it. We present the …
astrophysics, yet it remains unclear what physical mechanisms determine it. We present the …
Bonnsai: a Bayesian tool for comparing stars with stellar evolution models
FRN Schneider, N Langer, A de Koter, I Brott… - Astronomy & …, 2014 - aanda.org
Powerful telescopes equipped with multi-fibre or integral field spectrographs combined with
detailed models of stellar atmospheres and automated fitting techniques allow for the …
detailed models of stellar atmospheres and automated fitting techniques allow for the …
Variation of the high-mass slope of the stellar initial mass function: Theory meets observations
S Dib - The Astrophysical Journal, 2023 - iopscience.iop.org
We present observational evidence of a correlation between the high-mass slope of the
stellar initial mass function (IMF) in young star clusters and their stellar surface density, σ …
stellar initial mass function (IMF) in young star clusters and their stellar surface density, σ …
The influence of the environment on the spin evolution of low-mass stars–I. External photoevaporation of circumstellar discs
Massive stars are strong sources of far-ultraviolet radiation that can be hostile to the
evolution of protoplanetary discs, driving mass-loss by external photoevaporation and …
evolution of protoplanetary discs, driving mass-loss by external photoevaporation and …
The stellar IMF from isothermal MHD turbulence
We address the turbulent fragmentation scenario for the origin of the stellar initial mass
function (IMF), using a large set of numerical simulations of randomly driven supersonic …
function (IMF), using a large set of numerical simulations of randomly driven supersonic …
The evolution and properties of rotating massive star populations
J Choi, C Conroy, N Byler - The Astrophysical Journal, 2017 - iopscience.iop.org
We investigate the integrated properties of massive (> M 10) rotating single-star stellar
populations for a variety of initial rotation rates (= vv 0.0 crit, 0.2, 0.4, 0.5, and 0.6). We …
populations for a variety of initial rotation rates (= vv 0.0 crit, 0.2, 0.4, 0.5, and 0.6). We …