THE METALLICITY OF THE PLEIADES

David R. Soderblom; Tanmoy Laskar; Jeff A. Valenti; John R. Stauffer; Luisa M. Rebull

doi:10.1088/0004-6256/138/5/1292

THE METALLICITY OF THE PLEIADES

David R. Soderblom, Tanmoy Laskar, Jeff A. Valenti, John R. Stauffer, Luisa M. Rebull

Department of Physics

Research output: Contribution to journal › Article › peer-review

74 Citations (SciVal)

Abstract

We have measured the abundances of Fe, Si, Ni, Ti, and Na in 20 Pleiades stars with T eff values near solar and with low vsin i using high-resolution, high signal-to-noise echelle spectra. We have validated our procedures by also analyzing 10 field stars of a range of temperatures and metallicities that were observed by Valenti and Fischer. Our result for the Pleiades is [Fe/H] = +0.03 ± 0.02 ± 0.05 (statistical and systematic). The average of published measurements for the Pleiades is +0.042 ± 0.021.

Original language	English
Pages (from-to)	1292-1295
Number of pages	4
Journal	Astronomical Journal
Volume	138
Issue number	5
DOIs	https://doi.org/10.1088/0004-6256/138/5/1292
Publication status	Published - 1 Nov 2009

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10.1088/0004-6256/138/5/1292

http://stacks.iop.org/1538-3881/138/i=5/a=1292?key=crossref.f725c881be064634b5476b4f2d11902f

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title = "THE METALLICITY OF THE PLEIADES",

abstract = "We have measured the abundances of Fe, Si, Ni, Ti, and Na in 20 Pleiades stars with T eff values near solar and with low vsin i using high-resolution, high signal-to-noise echelle spectra. We have validated our procedures by also analyzing 10 field stars of a range of temperatures and metallicities that were observed by Valenti and Fischer. Our result for the Pleiades is [Fe/H] = +0.03 ± 0.02 ± 0.05 (statistical and systematic). The average of published measurements for the Pleiades is +0.042 ± 0.021.",

author = "Soderblom, \{David R.\} and Tanmoy Laskar and Valenti, \{Jeff A.\} and Stauffer, \{John R.\} and Rebull, \{Luisa M.\}",

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AU - Soderblom, David R.

AU - Laskar, Tanmoy

AU - Valenti, Jeff A.

AU - Stauffer, John R.

AU - Rebull, Luisa M.

PY - 2009/11/1

Y1 - 2009/11/1

N2 - We have measured the abundances of Fe, Si, Ni, Ti, and Na in 20 Pleiades stars with T eff values near solar and with low vsin i using high-resolution, high signal-to-noise echelle spectra. We have validated our procedures by also analyzing 10 field stars of a range of temperatures and metallicities that were observed by Valenti and Fischer. Our result for the Pleiades is [Fe/H] = +0.03 ± 0.02 ± 0.05 (statistical and systematic). The average of published measurements for the Pleiades is +0.042 ± 0.021.

AB - We have measured the abundances of Fe, Si, Ni, Ti, and Na in 20 Pleiades stars with T eff values near solar and with low vsin i using high-resolution, high signal-to-noise echelle spectra. We have validated our procedures by also analyzing 10 field stars of a range of temperatures and metallicities that were observed by Valenti and Fischer. Our result for the Pleiades is [Fe/H] = +0.03 ± 0.02 ± 0.05 (statistical and systematic). The average of published measurements for the Pleiades is +0.042 ± 0.021.

UR - https://www.scopus.com/pages/publications/70350613323

U2 - 10.1088/0004-6256/138/5/1292

DO - 10.1088/0004-6256/138/5/1292

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VL - 138

SP - 1292

EP - 1295

JO - Astronomical Journal

JF - Astronomical Journal

IS - 5

ER -

THE METALLICITY OF THE PLEIADES

Abstract

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