Comparison of alpha-element-enhanced simple stellar population models with Milky Way globular clusters

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dc.contributor.authorLee, H-C
dc.contributor.authorWorthey, G
dc.contributor.authorDotter, Aaron
dc.date.accessioned2015-12-13T22:48:47Z
dc.date.issued2009
dc.date.updated2016-02-24T09:42:30Z
dc.description.abstractWe present simple stellar population (SSP) models with scaled-solar and α-element-enhanced abundances. The SSP models are based on the Dartmouth Stellar Evolution Database, our library of synthetic stellar spectra, and a detailed systematic variation of
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/80221
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Abundances stars; Evolution stars; General stars; Globular clusters; Horizontal-branch
dc.titleComparison of alpha-element-enhanced simple stellar population models with Milky Way globular clusters
dc.typeJournal article
local.bibliographicCitation.issue5
local.bibliographicCitation.lastpage1454
local.bibliographicCitation.startpage1442
local.contributor.affiliationLee, H-C, Washington State University
local.contributor.affiliationWorthey, G, Washington State University
local.contributor.affiliationDotter, Aaron, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidDotter, Aaron, u5239381
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationf5625xPUB8513
local.identifier.citationvolume138
local.identifier.doi10.1088/0004-6256/138/5/1442
local.identifier.scopusID2-s2.0-70350614376
local.identifier.thomsonID000270852100019
local.type.statusPublished Version

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