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HIP 56948: A Solar Twin with a Low Lithium Abundance

Melendez Moreno, Jorge; Ramirez, Ivan

Description

For more than a decade, 18 Sco (HD 146233) has been considered the star that most closely resembles the Sun, even though significant differences such as its Li content, which is about 3 times solar, exist. Using high-resolution, high-S/N spectra obtained

dc.contributor.authorMelendez Moreno, Jorge
dc.contributor.authorRamirez, Ivan
dc.date.accessioned2015-12-07T22:30:57Z
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/22556
dc.description.abstractFor more than a decade, 18 Sco (HD 146233) has been considered the star that most closely resembles the Sun, even though significant differences such as its Li content, which is about 3 times solar, exist. Using high-resolution, high-S/N spectra obtained
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Stars: abundances; Stars: activity; Stars: atmospheres; Stars: fundamental parameters; Stars: individual (HIP 56948); Sun: fundamental parameters
dc.titleHIP 56948: A Solar Twin with a Low Lithium Abundance
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume669
dc.date.issued2007
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4362859xPUB22
local.type.statusPublished Version
local.contributor.affiliationMelendez Moreno, Jorge, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationRamirez, Ivan, University of Texas
local.description.embargo2037-12-31
local.bibliographicCitation.issue2 (November 10)
local.bibliographicCitation.startpageL89
local.bibliographicCitation.lastpageL92
local.identifier.doi10.1086/523942
dc.date.updated2015-12-07T10:10:48Z
local.identifier.scopusID2-s2.0-44849112317
CollectionsANU Research Publications

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