De re metallica: the cosmic chemical evolution of galaxies
The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …
abundances, their spatial distribution, and how these scale with various galactic properties …
Origin of the heaviest elements: The rapid neutron-capture process
JJ Cowan, C Sneden, JE Lawler, A Aprahamian… - Reviews of Modern …, 2021 - APS
The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
The origin of elements from carbon to uranium
To reach a deeper understanding of the origin of elements in the periodic table, we construct
Galactic chemical evolution (GCE) models for all stable elements from C (A= 12) to U (A …
Galactic chemical evolution (GCE) models for all stable elements from C (A= 12) to U (A …
First results from the IllustrisTNG simulations: A tale of two elements–chemical evolution of magnesium and europium
The distribution of elements in galaxies provides a wealth of information about their
production sites and their subsequent mixing into the interstellar medium. Here we …
production sites and their subsequent mixing into the interstellar medium. Here we …
Core-collapse supernovae from 9 to 120 solar masses based on neutrino-powered explosions
Nucleosynthesis, light curves, explosion energies, and remnant masses are calculated for a
grid of supernovae (SNe) resulting from massive stars with solar metallicity and masses from …
grid of supernovae (SNe) resulting from massive stars with solar metallicity and masses from …
From dawn till disc: Milky Way's turbulent youth revealed by the APOGEE+Gaia data
We use accurate estimates of aluminium abundance from the APOGEE Data Release 17
and Gaia Early Data Release 3 astrometry to select a highly pure sample of stars with …
and Gaia Early Data Release 3 astrometry to select a highly pure sample of stars with …
A grid of MARCS model atmospheres for late-type stars-I. Methods and general properties
B Gustafsson, B Edvardsson, K Eriksson… - Astronomy & …, 2008 - aanda.org
Context. In analyses of stellar spectra and colours, and for the analysis of integrated light
from galaxies, a homogeneous grid of model atmospheres of late-type stars and …
from galaxies, a homogeneous grid of model atmospheres of late-type stars and …
Presupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range− 3≤[Fe/H]≤ 0
M Limongi, A Chieffi - The Astrophysical Journal Supplement …, 2018 - iopscience.iop.org
Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars in the
Metallicity Range −3 ≤ [Fe/H] ≤ 0 - IOPscience This site uses cookies. By continuing to use …
Metallicity Range −3 ≤ [Fe/H] ≤ 0 - IOPscience This site uses cookies. By continuing to use …
Nucleosynthesis in stars and the chemical enrichment of galaxies
K Nomoto, C Kobayashi… - Annual Review of …, 2013 - annualreviews.org
After the Big Bang, production of heavy elements in the early Universe takes place starting
from the formation of the first stars, their evolution, and explosion. The first supernova …
from the formation of the first stars, their evolution, and explosion. The first supernova …
Star-formation histories, abundances, and kinematics of dwarf galaxies in the Local Group
E Tolstoy, V Hill, M Tosi - Annual Review of Astronomy and …, 2009 - annualreviews.org
Within the Local Universe galaxies can be studied in great detail star by star, and here we
review the results of quantitative studies in nearby dwarf galaxies. The color-magnitude …
review the results of quantitative studies in nearby dwarf galaxies. The color-magnitude …