Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

Experimental and theoretical radiative decay rates for highly excited ruthenium atomic levels and the solar abundance of ruthenium

Simple item page
dc.contributor.authorFivet, V
dc.contributor.authorQuinet, P
dc.contributor.authorPalmeri, P
dc.contributor.authorBiemont, E
dc.contributor.authorAsplund, Martin
dc.contributor.authorGrevesse, N
dc.contributor.authorSauval, A J
dc.contributor.authorEngstrom, L
dc.contributor.authorLundberg, H
dc.contributor.authorHartman, H
dc.contributor.authorNilsson, H
dc.date.accessioned2015-12-13T22:45:54Z
dc.date.issued2009
dc.date.updated2016-02-24T09:41:31Z
dc.description.abstractThe solar photospheric abundance of ruthenium is revised on the basis of a new set of oscillator strengths derived for Ru i transitions with wavelengths in the spectral range 2250-4710 Å. The new abundance value (in the usual logarithmic scale where the
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/80009
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Atomic data; Atomic processes; Sun: abundances
dc.titleExperimental and theoretical radiative decay rates for highly excited ruthenium atomic levels and the solar abundance of ruthenium
dc.typeJournal article
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage2132
local.bibliographicCitation.startpage2124
local.contributor.affiliationFivet, V, Universite de Mons-Hainaut
local.contributor.affiliationQuinet, P, Universite de Mons-Hainaut
local.contributor.affiliationPalmeri, P, Universite de Mons-Hainaut
local.contributor.affiliationBiemont, E, Universite de Mons-Hainaut
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationGrevesse, N, Universite de Liege
local.contributor.affiliationSauval, A J, Observatoire Royal de Belgique
local.contributor.affiliationEngstrom, L, Lund University
local.contributor.affiliationLundberg, H, Lund University
local.contributor.affiliationHartman, H, Lund University
local.contributor.affiliationNilsson, H, Lund University
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.ariespublicationf5625xPUB8350
local.identifier.citationvolume396
local.identifier.doi10.1111/j.1365-2966.2009.14761.x
local.identifier.scopusID2-s2.0-67649891988
local.type.statusPublished Version

Downloads

Original bundle

Now showing 1 - 1 of 1
Thumbnail Image
Name:
01_Fivet_Experimental_and_theoretical_2009.pdf
Size:
717.98 KB
Format:
Adobe Portable Document Format
Download

Collections

ANU Research Publications

DSpace software copyright © 2002-2026 LYRASIS