activity
20072026
most citedA Search for Stars of Very Low Metal Abundance. VI. Detailed Abundances of 313 Metal-Poor Stars

490 citations · 5.9k across the 130 of their papers we have counts for

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Showing 2012Show all

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astro-ph.SR2012★ 79 cited

Are There Any Stars Lacking Neutron-Capture Elements? Evidence from Strontium and Barium

Ian U. Roederer

The cosmic dispersion in the abundances of the heavy elements strontium and barium in halo stars is well known. Strontium and barium are detected in most cool, metal-poor giants, b…

astro-ph.SR2012★ 149 cited

New Hubble Space Telescope Observations of Heavy Elements in Four Metal-Poor Stars

Ian U. Roederer, James E. Lawler, Jennifer S. Sobeck +7

Elements heavier than the iron group are found in nearly all halo stars. A substantial number of these elements, key to understanding neutron-capture nucleosynthesis mechanisms, ca…

astro-ph.SR2012★ 55 cited

Germanium, Arsenic, and Selenium Abundances in Metal-Poor Stars

Ian U. Roederer

The elements germanium (Ge, Z=32), arsenic (As, Z=33), and selenium (Se, Z=34) span the transition from charged-particle or explosive synthesis of the iron-group elements to neutro…

astro-ph.SR2012★ 162 cited

Detection of Elements at All Three r-process Peaks in the Metal-Poor Star HD 160617

Ian U. Roederer, James E. Lawler

We report the first detection of elements at all three r-process peaks in the metal-poor halo star HD 160617. These elements include arsenic and selenium, which have not been detec…

astro-ph.SR2012★ 116 cited

RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system

G. Pietrzynski, I. B. Thompson, W. Gieren +14

RR Lyrae pulsating stars have been extensively used as tracers of old stellar populations for the purpose of determining the ages of galaxies, and as tools to measure distances to…

astro-ph.SR2012★ 85 cited

The double sub-giant branch of NGC 6656 (M22): a chemical characterization

A. F. Marino, A. P. Milone, C. Sneden +14

We present an abundance analysis of 101 subgiant branch (SGB) stars in the globular cluster M22. Using low resolution FLAMES/GIRAFFE spectra we have determined abundances of the ne…