Cluster melting: new, limiting, and liminal phenomena
Advances in Physics: X, 2018 The thermodynamic behaviour of clusters and nanoscale structures is both a challenge to the statistical basis of the theory, and of paramount importance to experiment.
Nicola Gaston
doaj +1 more source
Heavy Metal Rules. I. Exoplanet Incidence and Metallicity
Geosciences, 2019 The discovery of only a handful of exoplanets required establishing a correlation between giant planet occurrence and metallicity of their host stars.
Vardan Adibekyan
doaj +1 more source
Ca II TRIPLET SPECTROSCOPY OF SMALL MAGELLANIC CLOUD RED GIANTS. IV. ABUNDANCES FOR A LARGE SAMPLE OF FIELD STARS AND COMPARISON WITH THE CLUSTER SAMPLE [PDF]
, 2016 This paper represents a major step forward in the systematic and homogeneous study of Small Magellanic Cloud (SMC) star clusters and field stars carried out by applying the calcium triplet technique.
Carraro, Giovanni +5 more
core +1 more source
The MOSDEF Survey: A Stellar Mass–SFR–Metallicity Relation Exists at z ∼ 2.3 [PDF]
, 2017 We investigate the nature of the relation among stellar mass, star formation rate, and gas-phase metallicity (the –SFR–Z relation) at high redshifts using a sample of 260 star-forming galaxies at z ∼ 2.3 from the MOSDEF survey.
R. Sanders +17 more
semanticscholar +1 more source
Nearby supernova host galaxies from the CALIFA Survey: II. SN environmental metallicity [PDF]
, 2016 The metallicity of a supernova (SN) progenitor, together with its mass, is one of the main parameters that rules their outcome.
Badenes, C. +18 more
core +9 more sources
Similar star formation rate and metallicity variability time-scales drive the fundamental metallicity relation [PDF]
, 2017 The fundamental metallicity relation (FMR) is a postulated correlation between galaxy stellar mass, star formation rate (SFR), and gas-phase metallicity.
P. Torrey +19 more
semanticscholar +1 more source
Chemodynamic evolution of dwarf galaxies in tidal fields [PDF]
, 2016 The mass-metallicity relation shows that the galaxies with the lowest mass have the lowest metallicities. As most dwarf galaxies are in group environments, interaction effects such as tides could contribute to this trend.
Martel, Hugo +2 more
core +2 more sources
Massive black hole binaries from runaway collisions: the impact of metallicity [PDF]
, 2016 The runaway collision scenario is one of the most promising mechanisms to explain the formation of intermediate-mass black holes (IMBHs) in young dense star clusters.
M. Mapelli
semanticscholar +1 more source
Galaxy metallicity scaling relations in the EAGLE simulations [PDF]
, 2017 We quantify the correlations between gas-phase and stellar metallicities and global properties of galaxies, such as stellar mass, halo mass, age and gas fraction, in the Evolution and Assembly of GaLaxies and their Environments suite of cosmological ...
M. Rossi +4 more
semanticscholar +1 more source
The cosmic evolution of dust-corrected metallicity in the neutral gas [PDF]
, 2017 Interpreting abundances of Damped Ly-$\alpha$ Absorbers (DLAs) from absorption-line spectroscopy has typically been a challenge because of the presence of dust.
A. D. Cia +3 more
semanticscholar +1 more source