Lithium isotopic abundances in stars

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dc.contributor.authorNissen, Poul E
dc.contributor.authorAsplund, Martin
dc.coverage.spatialAveiro Portugal
dc.date.accessioned2015-12-10T22:36:31Z
dc.date.createdSeptember 11-15 2006
dc.date.issued2008
dc.date.updated2015-12-09T10:36:23Z
dc.description.abstractThe Li isotope ratio, 6Li/7Li, in stars can be determined from the isotopic shift in the Li I 670.8 nm resonance line. Because of the small effect this however requires truly precision spectroscopy: spectral resolving power R ≥ 105 and S/N ≥ 500. In t
dc.identifier.isbn9783540754848
dc.identifier.urihttp://hdl.handle.net/1885/56698
dc.publisherSpringer-Verlag Berlin Heidelberg
dc.relation.ispartofseriesPrecision Spectroscopy in Astrophysics
dc.sourcePrecision Spectroscopy in Astrophysics
dc.titleLithium isotopic abundances in stars
dc.typeConference paper
local.bibliographicCitation.lastpage8
local.bibliographicCitation.startpage3
local.contributor.affiliationNissen, Poul E, University of Aarhus
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.authoremailu4042723@anu.edu.au
local.contributor.authoruidAsplund, Martin, u4042723
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationU3488905xPUB372
local.identifier.doi10.1007/978-3-540-75485-5_1
local.identifier.scopusID2-s2.0-36448944774
local.identifier.uidSubmittedByU3488905
local.type.statusPublished Version

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