Search Results - "Stanford, Laura M."

A Chemical Signature from Fast-rotating Low-metallicity Massive Stars: ROA 276 in ω Centauri by Yong, David, Norris, John E., Costa, Gary S. Da, Stanford, Laura M., Karakas, Amanda I., Shingles, Luke J., Hirschi, Raphael, Pignatari, Marco

“…We present a chemical abundance analysis of a metal-poor star, ROA 276, in the stellar system ω Centauri. We confirm that this star has an unusually high…”
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Abundances of C, N, Sr, and Ba on the Red Giant Branch of ω Centauri by Stanford, Laura M, Da Costa, G. S, Norris, John E

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Two groups within the thick disc of the Milky Way? by Stanford, Laura M., Lambert, David L.

“…Abstract Compositions of F and G dwarf stars in two groups of thick disc stars are presented. The groups identified by Schuster et al. have mean…”
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The Age and Metallicity Relation of ω Centauri by Stanford, Laura M, Da Costa, Gary S, Norris, John E, Cannon, Russell D

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Abundances on the Main Sequence of ω Centauri by Stanford, Laura M, Da Costa, G. S, Norris, John E, Cannon, Russell D

“…Abundance ratios of carbon, nitrogen, and strontium relative to iron, calculated using spectrum synthesis techniques, are given for a sample of main-sequence…”
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A Sr-rich Star on the Main Sequence of ω Centauri by Stanford, Laura M, Da Costa, G. S, Norris, John E, Cannon, Russell D

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A Chemical Signature from Fast-rotating Low-metallicity Massive Stars: ROA 276 in Centauri This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile by Yong, David, Norris, John E., Costa, Gary S. Da, Stanford, Laura M., Karakas, Amanda I., Shingles, Luke J., Hirschi, Raphael, Pignatari, Marco

“…We present a chemical abundance analysis of a metal-poor star, ROA 276, in the stellar system Centauri. We confirm that this star has an unusually high [Sr/Ba]…”
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ABUNDANCES OF C, N, Sr, AND Ba ON THE RED GIANT BRANCH OF Delta w CENTAURI by Stanford, Laura M, Da Costa, G S, Norris, John E

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ABUNDANCES OF C, N, Sr, AND Ba ON THE RED GIANT BRANCH OF {omega} CENTAURI by Stanford, Laura M., Da Costa, G. S., Norris, John E.

“…Abundances relative to iron for carbon, nitrogen, strontium, and barium are presented for 33 stars on the red giant branch (RGB) of the globular cluster…”
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A chemical signature from fast-rotating low-metallicity massive stars: ROA 276 in omega Centauri by Yong, David, Norris, John E, Da Costa, Gary S, Stanford, Laura M, Karakas, Amanda I, Shingles, Luke J, Hirschi, Raphael, Pignatari, Marco

“…We present a chemical abundance analysis of a metal-poor star, ROA 276, in the stellar system omega Centauri. We confirm that this star has an unusually high…”
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Carbon in the Draco Dwarf Spheroidal Galaxy by Shetrone, Matthew D, Smith, Graeme H, Stanford, Laura M, Siegel, Michael H, Bond, Howard E

“…AJ 2013 Measurements of [C/Fe], [Ca/H], and [Fe/H] have been derived from Keck I LRISb spectra of 35 giants in the Draco dwarf spheroidal galaxy. The iron…”
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Abundances of C, N, Sr and Ba on the red giant branch of omega Centauri by Stanford, Laura M, Da Costa, Gary S, Norris, John E

“…Abundances relative to iron for carbon, nitrogen, strontium and barium are presented for 33 stars on the red giant branch of the globular cluster omega…”
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Optical Spectra of Flat-Spectrum ICRF Radio Sources by Titov, Oleg, Stanford, Laura M, Johnston, Helen M, Pursimo, Tapio, Hunstead, Richard W, Jauncey, David L, Maslennikov, K, Boldycheva, A

“…Continuing our program of spectroscopic observations of ICRF sources, we present redshifts for 120 quasars and radio galaxies. Data were obtained with five…”
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Abundances on the Main Sequence of Omega Centauri by Stanford, Laura M, Da Costa, G. S, Norris, John E

“…Abundance ratios of carbon, nitrogen and strontium relative to iron, calculated using spectrum synthesis techniques, are given for a sample of main sequence…”
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A Sr-Rich Star on the Main Sequence of Omega Centauri by Stanford, Laura M, Da Costa, G. S, Norris, John E, Cannon, Russell D

“…Astrophys.J.653:L117-L120,2006 Abundance ratios relative to iron for carbon, nitrogen, strontium and barium are presented for a metal-rich main sequence star…”
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