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dc.contributorVirginia Tech
dc.contributor.authorPalmeri, P.
dc.contributor.authorQuinet, P.
dc.contributor.authorMendoza, C.
dc.contributor.authorBautista, M. A.
dc.contributor.authorGarcia, J.
dc.contributor.authorWitthoeft, M. C.
dc.contributor.authorKallman, T. R.
dc.date.accessioned2014-03-10T13:18:51Z
dc.date.available2014-03-10T13:18:51Z
dc.date.issued2008-12
dc.identifier.citationP. Palmeri et al. 2008 ApJS 179 542 doi:10.1086/591965
dc.identifier.issn0067-0049
dc.identifier.urihttp://hdl.handle.net/10919/25851
dc.description.abstractRadiative and Auger decay data have been calculated for modeling the K lines in ions of the nickel isonuclear sequence, from Ni(+) up to Ni(27+). Level energies, transition wavelengths, radiative transition probabilities, and radiative and Auger widths have been determined using Cowan's Hartree-Fock with relativistic corrections (HFR) method. Auger widths for the third-row ions (Ni(+)-Ni(10+)) have been computed using single-configuration average (SCA) compact formulae. Results are compared with data sets computed with the AUTOSTRUCTURE and MCDF atomic structure codes and with available experimental and theoretical values, mainly in highly ionized ions and in the solid state.
dc.description.sponsorshipNASA Astronomy and Physics Research and Analysis Program
dc.language.isoen_US
dc.publisherIOP PUBLISHING LTD
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjectatomic data
dc.subjectatomic processes
dc.subjectline: formation
dc.subjectx-rays: general
dc.subjectray-intensity ratios
dc.subjecttransition-probability ratios
dc.subjectxmm-newton
dc.subjectvacancy
dc.subjectstates
dc.subjectabsorption features
dc.subjectigr j16318-4848
dc.subjectenergy-levels
dc.subjectvela x-1
dc.subjectfe-xvii
dc.subjectemission
dc.titleRadiative and Auger Decay Data for Modeling Nickel K Lines
dc.typeArticle - Refereed
dc.contributor.departmentPhysicsen_US
dc.identifier.urlhttp://iopscience.iop.org/0067-0049/179/2/542
dc.date.accessed2014-02-28
dc.title.serialAstrophysical Journal Supplement Series
dc.identifier.doihttps://doi.org/10.1086/591965


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