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Magnesium Isotope Ratios in Hyades Stars

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dc.contributor.authorYong, David
dc.contributor.authorLambert, D.L.
dc.contributor.authorPrieto, Carlos Allende
dc.contributor.authorPaulson, D.B.
dc.date.accessioned2015-12-08T22:24:59Z
dc.date.issued2004
dc.date.updated2015-12-08T09:01:12Z
dc.description.abstractUsing classical model atmospheres and an LTE analysis, Mg isotope ratios 24Mg: 25Mg: 26Mg are measured in 32 Hyades dwarfs covering effective temperatures 4000 K ≤ T eff ≤ 5000 K. We find no significant trend in any isotope ratio versus T eff, and the
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/33222
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Open clusters and associations: individual (Hyades); Stars: abundances; Stars: atmospheres
dc.titleMagnesium Isotope Ratios in Hyades Stars
dc.typeJournal article
local.bibliographicCitation.lastpage707
local.bibliographicCitation.startpage697
local.contributor.affiliationYong, David, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLambert, D.L., University of Texas
local.contributor.affiliationPrieto, Carlos Allende, University of Texas
local.contributor.affiliationPaulson, D.B., University of Michigan
local.contributor.authoruidYong, David, u3207952
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3379551xPUB100
local.identifier.citationvolume603
local.identifier.doi10.1086/381701
local.identifier.scopusID2-s2.0-2142699436
local.type.statusPublished Version

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