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19992023
most citedThe Galactic Thick Disk Stellar Abundances

422 citations · 4.4k across the 64 of their papers we have counts for

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Showing 2013 · astro-ph.GAShow all

5 papers · 2 filters

astro-ph.GA2013★ 207 cited

Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] < -2

Judith Cohen, Norbert Christlieb, Ian Thompson +5

From detailed abundance analysis of >100 Hamburg/ESO candidate extremely metal-poor (EMP) stars we find 45 with [Fe/H] < -3.0 dex. We identify a heretofore unidentified group: Ca-d…

astro-ph.GA2013★ 186 cited

Chemistry of the Sagittarius Dwarf Galaxy: a Top-Light IMF, Outflows and the R-Process

Andrew McWilliam, George Wallerstein, Marta Mottini

From chemical abundance analysis of stars in the Sagittarius dwarf spheroidal galaxy (Sgr), we conclude that the alpha-element deficiencies cannot be due to the Type Ia supernova (…

astro-ph.GA2013★ 21 cited

Chemical Abundance Evidence of Enduring High Star Formation Rates in an Early Type Galaxy: High [Ca/Fe] in NGC 5128 Globular Clusters

J. E. Colucci, M. F. Duran, R. A. Bernstein +1

We present [Fe/H], ages, and Ca abundances for an initial sample of 10 globular clusters in NGC 5128 obtained from high resolution, high signal-to-noise ratio echelle spectra of th…

astro-ph.GA2013★ 36 cited

Spectrum Syntheses of High Resolution Integrated Light Spectra of Galactic Globular Clusters

Charli M. Sakari, Matthew Shetrone, Kim Venn +2

Spectrum syntheses for three elements (Mg, Na, and Eu) in high-resolution integrated light spectra of the Galactic globular clusters 47 Tuc, M3, M13, NGC 7006, and M15 are presente…

astro-ph.GA2013★ 41 cited

A comprehensive chemical abundance study of the outer halo globular cluster M 75

Nikolay Kacharov, Andreas Koch, Andrew McWilliam

Context: M 75 is a relatively young Globular Cluster (GC) found at 15 kpc from the Galactic centre at the transition region between the inner and outer Milky Way halos. Aims: Our a…