Results 11 to 20 of about 625,053 (333)

The mass–metallicity and the fundamental metallicity relation revisited on a fully Te-based abundance scale for galaxies [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2019
The relationships between stellar mass, gas-phase metallicity and star-formation rate (i.e. the mass–metallicity, MZR, and the fundamental metallicity relation, FMR) in the local Universe are revisited by fully anchoring the metallicity determination ...
M. Curti   +3 more
semanticscholar   +1 more source

Inducing metallicity in graphene nanoribbons via zero-mode superlattices [PDF]

open access: yesScience, 2019
Making metallic ribbons In its usual two-dimensional form, graphene does not have an energy gap in its electronic structure. However, one-dimensional ribbons made of the material are semiconducting and making them metallic is tricky.
Daniel J. Rizzo   +9 more
semanticscholar   +1 more source

Massive Star Formation in Metal-Enriched Haloes at High Redshift

open access: yesThe Open Journal of Astrophysics, 2020
The formation of supermassive stars has generally been studied under the assumption of rapid accretion of pristine metal-free gas. Recently it was found, however, that gas enriched to metallicities up to Z + 10^-3 Solar can also facilitate supermassive ...
Zoltán Haiman   +3 more
doaj   +1 more source

The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
Six gravitational wave events have been reported by the LIGO-Virgo collaboration (LVC), five of them associated with black hole binary (BHB) mergers and one with a double neutron star (DNS) merger, while the coalescence of a black hole-neutron star (BHNS)
N. Giacobbo, M. Mapelli
semanticscholar   +1 more source

The influence of metallicity on helium and CO core masses in massive stars [PDF]

open access: yesSerbian Astronomical Journal, 2023
We present the results of 58 detailed evolutionary models of massive single stars and close binary systems with the Solar and Small Magellanic Cloud (SMC) metallicity computed with the MESA (Modules for Experiments in Stellar Astrophysics ...
Petrović Jelena
doaj   +1 more source

Grids of stellar models with rotation - I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014) [PDF]

open access: yes, 2011
Aims. Many topical astrophysical research areas, such as the properties of planet host stars, the nature of the progenitors of different types of supernovae and gamma ray bursts, and the evolution of galaxies, require complete and homogeneous sets of ...
S. Ekstrom   +11 more
semanticscholar   +1 more source

The Effect of Metallicity on the Nonequilibrium Abundance of Hydrogen-dominated Exoplanet Atmospheres

open access: yesThe Astrophysical Journal, 2023
The atmospheric metallicity greatly influences the composition of exoplanet atmospheres. The effect of metallicity on the thermochemical equilibrium is well studied, though its effect on the disequilibrium abundance is loosely constrained. In this study,
Vikas Soni, Kinsuk Acharyya
doaj   +1 more source

Metal Preferences and Metallation [PDF]

open access: yesJournal of Biological Chemistry, 2014
The metal binding preferences of most metalloproteins do not match their metal requirements. Thus, metallation of an estimated 30% of metalloenzymes is aided by metal delivery systems, with ∼ 25% acquiring preassembled metal cofactors. The remaining ∼ 70% are presumed to compete for metals from buffered metal pools.
Foster, Andrew W.   +2 more
openaire   +4 more sources

Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity [PDF]

open access: yes, 2000
We present analytic formulae that approximate the evolution of stars for a wide range of mass M and metallicity Z. Stellar luminosity, radius and core mass are given as a function of age, M and Z, for all phases from the zero-age main sequence up to, and
J. Hurley, O. Pols, C. Tout
semanticscholar   +1 more source

Resolving the Metallicity Distribution of the Stellar Halo with the H3 Survey [PDF]

open access: yesAstrophysical Journal, 2019
The Galactic stellar halo is predicted to have formed at least partially from the tidal disruption of accreted dwarf galaxies. This assembly history should be detectable in the orbital and chemical properties of stars.
C. Conroy   +6 more
semanticscholar   +1 more source

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