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The Hamburg/ESO R-process Enhanced Star Survey (HERES) I. Project description, and discovery of two stars with strong enhancements of neutron-capture elements

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dc.contributor.authorChristlieb, Norbert
dc.contributor.authorBeers, Timothy C
dc.contributor.authorBarklem, Paul S
dc.contributor.authorBessell, Michael
dc.contributor.authorHill, V
dc.contributor.authorHolmberg, Johan
dc.contributor.authorKorn, A J
dc.contributor.authorMarstellar, B
dc.contributor.authorMashonkina, L
dc.contributor.authorQian, Y-Z
dc.contributor.authorRossi, Silvia
dc.contributor.authorWasserburg, G J
dc.contributor.authorZickgraf, F-J
dc.contributor.authorKratz, K-L
dc.contributor.authorNordstrom, B
dc.contributor.authorPfeiffer, B
dc.contributor.authorRhee, Jaehyon
dc.contributor.authorRyan, Sean G
dc.date.accessioned2015-12-13T23:11:24Z
dc.date.available2015-12-13T23:11:24Z
dc.date.issued2004
dc.date.updated2015-12-12T08:27:23Z
dc.description.abstractWe report on a dedicated effort to identify and study metal-poor stars strongly enhanced in r-process elements ([r/Fe] > 1 dex; hereafter r-II stars), the Hamburg/ESO R-process Enhanced Star survey (HERES). Moderate-resolution (∼2 Å) follow-up spectros
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/87583
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Absorption; Astronomy; Chronometers; Isotopes; Neutrons; Spectroscopy; Statistical methods; Abundance-stars; Abundances-galaxy; Halo; Population II; Surveys-stars; Galaxies Galaxy: abundances; Galaxy: halo; Stars: abundances; Stars: population II; Surveys
dc.titleThe Hamburg/ESO R-process Enhanced Star Survey (HERES) I. Project description, and discovery of two stars with strong enhancements of neutron-capture elements
dc.typeJournal article
local.bibliographicCitation.lastpage1037
local.bibliographicCitation.startpage1027
local.contributor.affiliationChristlieb, Norbert, University of Hamburg
local.contributor.affiliationBeers, Timothy C, Michigan State University
local.contributor.affiliationBarklem, Paul S, Uppsala Astronomical Observatory
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationHill, V, Observatoire de Paris
local.contributor.affiliationHolmberg, Johan, Tuorla Observatory
local.contributor.affiliationKorn, A J, Uppsala Astronomical Observatory
local.contributor.affiliationMarstellar, B, Michigan State University
local.contributor.affiliationMashonkina, L, Universitatssternwarte Munchen
local.contributor.affiliationQian, Y-Z, University of Minnesota
local.contributor.affiliationRossi, Silvia, Universidade de Sao Paulo
local.contributor.affiliationWasserburg, G J, California Institute of Technology
local.contributor.affiliationZickgraf, F-J, University of Hamburg
local.contributor.affiliationKratz, K-L, Johannes Gutenberg University of Mainz
local.contributor.affiliationNordstrom, B, Lund University
local.contributor.affiliationPfeiffer, B, Johannes Gutenberg University of Mainz
local.contributor.affiliationRhee, Jaehyon, Yonsei University
local.contributor.affiliationRyan, Sean G, Open University
local.contributor.authoruidBessell, Michael, u6900904
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16932
local.identifier.citationvolume428
local.identifier.doi10.1051/0004-6361:20041536
local.identifier.scopusID2-s2.0-19944411789
local.type.statusPublished Version

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