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
Metallicity-dependent signatures in the Kepler planets [PDF]
Monthly notices of the Royal Astronomical Society, 2018 Using data from the California-Kepler-Survey (CKS) we study trends in planetary properties with host star metallicity for close-in planets. By incorporating knowledge of the properties of the planetary radius gap identified by the CKS survey, we are able
J. Owen, R. Murray-Clay
semanticscholar +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
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
F stars, metallicity, and the ages of red galaxies at z > 1 [PDF]
, 2001 We explore whether the rest-frame near-UV spectral region, observable in high-redshift galaxies via optical spectroscopy, contains sufficient information to allow the degeneracy between age and metallicity to be lifted.
A. F. Heavens +37 more
core +3 more sources
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
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
Stellar population gradients from cosmological simulations: dependence on mass and environment in local galaxies [PDF]
, 2010 The age and metallicity gradients for a sample of group and cluster galaxies from N-body+hydrodynamical simulation are analyzed in terms of galaxy stellar mass.
A. D. Romeo +41 more
core +1 more source
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
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