Results 21 to 30 of about 699,213 (384)

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

The Close Binary Fraction of Solar-type Stars Is Strongly Anticorrelated with Metallicity [PDF]

open access: yesAstrophysical Journal, 2018
There is now strong evidence that the close binary fraction (P < 104 days; a < 10 au) of solar-type stars (M1 ≈ 0.6–1.5 ) decreases significantly with metallicity. Although early surveys showed that the observed spectroscopic binary (SB) fractions in the
M. Moe, K. Kratter, C. Badenes
semanticscholar   +1 more source

A Surprising Lack of Metallicity Evolution with Redshift in the Long Gamma-Ray Burst Host Galaxy Population

open access: yesThe Astrophysical Journal, 2023
The number of long-duration gamma-ray burst (LGRB) host galaxies with measured metallicities and host masses has expanded sufficiently to investigate how the distributions of these properties change with redshift.
J. F. Graham, P. Schady, A. S. Fruchter
doaj   +1 more source

Metallicity Calibrations and the Mass-Metallicity Relation for Star-forming Galaxies [PDF]

open access: yes, 2008
We investigate the effect of metallicity calibrations, AGN classification, and aperture covering fraction on the local mass-metallicity (M-Z) relation using 27,730 star-forming galaxies from the SDSS Data Release 4.
L. Kewley, S. Ellison
semanticscholar   +1 more source

THE STUDY OF GALACTIC BEAT CEPHEIDS WITH APPLICATION OF ITS RESULTS TO THOSE IN THE MAGELLANIC CLOUDS

open access: yesOdessa Astronomical Publications, 2014
A thorough study of the correlation between P1=P0 ratio, fundamental period, and chemical composition (abundances of metals that compose Z) was conducted to investigate the significance of the iron-peak elements on the ratio. The results suggested a more
F. A. Chekhonadskikh   +2 more
doaj   +1 more source

Metallicity and Superconductivity in Doped Strontium Titanate [PDF]

open access: yesAnnual Review of Condensed Matter Physics, 2018
Strontium titanate is a wide-gap semiconductor avoiding a ferroelectric instability thanks to quantum fluctuations. This proximity leads to strong screening of static Coulomb interaction and paves the way for the emergence of a very dilute metal with ...
C. Collignon   +4 more
semanticscholar   +1 more source

Metal–metal bonded compounds and metal clusters [PDF]

open access: yesInorganica Chimica Acta, 2015
Preface.
Falvello, Larry R., Murillo, Carlos A.
openaire   +2 more sources

High-resolution Spectroscopic Metallicities of Milky Way Cepheid Standards and Their Impact on the Leavitt Law and the Hubble Constant

open access: yesThe Astrophysical Journal Letters, 2023
Milky Way Cepheid variables with accurate Hubble Space Telescope photometry have been established as standards for primary calibration of the cosmic distance ladder to achieve a percent-level determination of the Hubble constant ( H _0 ).
Anupam Bhardwaj   +12 more
doaj   +1 more source

Slater-Pauling behavior and origin of the half-metallicity of the full-Heusler alloys [PDF]

open access: yes, 2002
Using the full-potential screened Korringa-Kohn-Rostoker method we study the full-Heusler alloys based on Co, Fe, Rh, and Ru. We show that many of these compounds show a half-metallic behavior; however, in contrast to the half-Heusler alloys the energy ...
I. Galanakis   +2 more
semanticscholar   +1 more source

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