The cosmological star formation history from the Local Cosmological Volume of galaxies and constraints on the matter homogeneity

M Haslbauer, P Kroupa… - Monthly Notices of the …, 2023 - academic.oup.com
ABSTRACT The Lilly–Madau plot is commonly interpreted as the history of the cosmic star
formation of the Universe by showing the co-moving star formation rate density (SFRD) over …

Neutrino Heating in 1D, 2D, and 3D core-collapse supernovae: characterizing the explosion of high-compactness stars

L Boccioli, D Vartanyan, EP O'Connor… - arXiv preprint arXiv …, 2025 - arxiv.org
Massive stars can end their lives with a successful supernova explosion (leaving behind a
neutron star or, more rarely, a black hole), or a failed explosion that leaves behind a black …

The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars are Metal-Rich

JW Johnson, DH Weinberg, GA Blanc… - arXiv preprint arXiv …, 2024 - arxiv.org
Metallicities of both gas and stars decline toward large radii in spiral galaxies, a trend known
as the radial metallicity gradient. We quantify the evolution of the metallicity gradient in the …

[PDF][PDF] Open Clusters as Tracers of Galactic Chemical Evolution

K Boucher - 2024 - ir.canterbury.ac.nz
Open Clusters as Tracers of Galactic Chemical Evolution Page 1 School of Physical and
Chemical Sciences Open Clusters as Tracers of Galactic Chemical Evolution by Kyle Boucher …

The initial mass function of stars

P Kroupa, E Gjergo, T Jerabkova, Z Yan - arXiv preprint arXiv:2410.07311, 2024 - arxiv.org
The initial mass function (IMF) is one of the most important functions in astrophysics because
it is key to reconstructing the cosmological matter cycle, understanding the formation of …