139 citations · 337 across the 7 of their papers we have counts for
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Why is the Main Sequence of NGC 2482 So Fat?
Kevin Krisciunas, Nicholas B. Suntzeff, Daniel Q. Nagasawa +3
We present the results of high resolution spectra of seven stars in the field of NGC 2482, an open star cluster of age 447 Myr. We confirm the previously published values of the ra…
Chemical Abundance Analysis of Three -Poor, Metal-Poor Stars in the Ultra-Faint Dwarf Galaxy Horologium I
D. Q. Nagasawa, J. L. Marshall, J. D. Simon +68
We present chemical abundance measurements of three stars in the ultra-faint dwarf galaxy Horologium I, a Milky Way satellite discovered by the Dark Energy Survey. Using high resol…
An R-process enhanced star in the dwarf galaxy Tucana III
T. T. Hansen, J. D. Simon, J. L. Marshall +48
Chemically peculiar stars in dwarf galaxies provide a window for exploring the birth environment of stars with varying chemical enrichment. We present a chemical abundance analysis…