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Spectroscopic Studies of Extremely Metal-Poor Stars with the SUBARU High Dispersion Spectrograph I. Observational Data

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dc.contributor.authorHonda, Satoshi
dc.contributor.authorAoki, Wako
dc.contributor.authorAnderson, W G
dc.contributor.authorIzumiura, Hideyuki
dc.contributor.authorKajino, Toshitaka
dc.contributor.authorKambe, Eiji
dc.contributor.authorKawanomoto, Satoshi
dc.contributor.authorNoguchi, Kunio
dc.contributor.authorOkita, Kiichi
dc.contributor.authorSadakane, Kozo
dc.contributor.authorSato, Bun'ei
dc.contributor.authorTakada-Hidai, Masahide
dc.contributor.authorTakeda, Yoichi
dc.contributor.authorWatanabe, Etsuji
dc.contributor.authorBeers, Timothy C
dc.contributor.authorNorris, John
dc.contributor.authorRyan, Sean G
dc.date.accessioned2015-12-13T23:10:11Z
dc.date.available2015-12-13T23:10:11Z
dc.date.issued2004
dc.date.updated2015-12-12T08:22:51Z
dc.description.abstractWe have obtained high-resolution (R ≃ 50,000 or 90,000), high-quality (S/N ≳ 100) spectra of 22 very metal-poor stars ([Fe/H] ≲ - 2.5) with the High Dispersion Spectrograph fabricated for the 8.2 m Subaru Telescope. The spectra cover the wavelength
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/87341
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Nuclear reactions; Nucleosynthesis, abundances; Stars: abundances; Stars: Population II
dc.titleSpectroscopic Studies of Extremely Metal-Poor Stars with the SUBARU High Dispersion Spectrograph I. Observational Data
dc.typeJournal article
local.bibliographicCitation.lastpage128
local.bibliographicCitation.startpage113
local.contributor.affiliationHonda, Satoshi, National Astronomical Observatory of Japan
local.contributor.affiliationAoki, Wako, National Astronomical Observatory of Japan
local.contributor.affiliationAnderson, W G, University of Texas
local.contributor.affiliationIzumiura, Hideyuki, National Astronomical Observatory of Japan
local.contributor.affiliationKajino, Toshitaka, National Astronomical Observatory of Japan
local.contributor.affiliationKambe, Eiji, National Defence Academy
local.contributor.affiliationKawanomoto, Satoshi, National Astronomical Observatory of Japan
local.contributor.affiliationNoguchi, Kunio, National Astronomical Observatory of Japan
local.contributor.affiliationOkita, Kiichi, National Astronomical Observatory of Japan
local.contributor.affiliationSadakane, Kozo, Osaka Kyoiku University
local.contributor.affiliationSato, Bun'ei, National Astronomical Observatory of Japan
local.contributor.affiliationTakada-Hidai, Masahide, Tokai University
local.contributor.affiliationTakeda, Yoichi, National Astronomical Observatory of Japan
local.contributor.affiliationWatanabe, Etsuji, National Astronomical Observatory of Japan
local.contributor.affiliationBeers, Timothy C, Michigan State University
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationRyan, Sean G, Open University
local.contributor.authoruidNorris, John, u7401084
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16583
local.identifier.citationvolume152
local.identifier.doi10.1086/383201
local.identifier.scopusID2-s2.0-2442690410
local.type.statusPublished Version

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