View Item 

Show simple item record

Energy levels and transition probabilities in doubly-ionized erbium (Er III)

dc.contributor.authorWyart, Jean-Françoisen_US
dc.contributor.authorBlaise, Jeanen_US
dc.contributor.authorBidelman, William P.en_US
dc.contributor.authorCowley, Charles R.en_US
dc.date.accessioned2006-12-19T19:25:29Z
dc.date.available2006-12-19T19:25:29Z
dc.date.issued1997-11-01en_US
dc.identifier.citationWyart, Jean-François; Blaise, Jean; Bidelman, William P; Cowley, Charles R (1997). "Energy levels and transition probabilities in doubly-ionized erbium (Er III)." Physica Scripta. 56(5): 446-458. <http://hdl.handle.net/2027.42/49231>en_US
dc.identifier.issn1402-4896en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/49231
dc.description.abstractThe spectrum of Er III reported by Becher (1966) was reanalysed with the support of new predictions of energies and transition probabilities. The number of energy levels was increased from 45 to 115, including two levels of 4f117s and the levels 3F3, 3F2 and 1G4 of the ground configuration 4f12. All 470 classified lines are reported with transition probabilities for most of them. Several of these lines had not yet been attributed to Er III in the spectrum of the star HR465.en_US
dc.format.extent3118 bytes
dc.format.extent1074978 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherIOP Publishing Ltden_US
dc.titleEnergy levels and transition probabilities in doubly-ionized erbium (Er III)en_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, Ann Arbor, MI 48109-1090, USAen_US
dc.contributor.affiliationotherLaboratoire Aimé Cotton, Bât. 505, CNRS II, Centre universitaire, F-91405, Orsay, Franceen_US
dc.contributor.affiliationotherLaboratoire Aimé Cotton, Bât. 505, CNRS II, Centre universitaire, F-91405, Orsay, Franceen_US
dc.contributor.affiliationotherDepartment of Astronomy, Case Western Reserve University, Cleveland, OH 44106-7215, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/49231/2/physscr_56_5_008.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1088/0031-8949/56/5/008en_US
dc.identifier.sourcePhysica Scripta.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Name:
physscr_56_5_008.pdf
Size:
1.025MB
Format:
PDF
View/Open

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.