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dc.contributorVirginia Techen
dc.contributor.authorGarcia, J.en
dc.contributor.authorKallman, T. R.en
dc.contributor.authorWitthoeft, M.en
dc.contributor.authorBehar, E.en
dc.contributor.authorMendoza, C.en
dc.contributor.authorPalmeri, P.en
dc.contributor.authorQuinet, P.en
dc.contributor.authorBautista, M. A.en
dc.contributor.authorKlapisch, M.en
dc.date.accessioned2014-03-10T13:18:50Zen
dc.date.available2014-03-10T13:18:50Zen
dc.date.issued2009-12en
dc.identifier.citationJ. García et al. 2009 ApJS 185 477 doi:10.1088/0067-0049/185/2/477en
dc.identifier.issn0067-0049en
dc.identifier.urihttp://hdl.handle.net/10919/25847en
dc.description.abstractReliable atomic data have been computed for the spectral modeling of the nitrogen K lines, which may lead to useful astrophysical diagnostics. Data sets comprise valence and K-vacancy level energies, wavelengths, Einstein A-coefficients, radiative and Auger widths, and K-edge photoionization cross sections. An important issue is the lack of measurements that are usually employed to fine-tune calculations so as to attain spectroscopic accuracy. In order to estimate data quality, several atomic structure codes are used and extensive comparisons with previous theoretical data have been carried out. In the calculation of K photoabsorption with the Breit-Pauli R-matrix method, both radiation and Auger dampings, which cause the smearing of the K edge, are taken into account. This work is part of a wider project to compute atomic data in the X-ray regime to be included in the database of the popular XSTAR modeling code.en
dc.description.sponsorshipNASA 08-ADP08-0076en
dc.language.isoen_USen
dc.publisherIOP PUBLISHING LTDen
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjectatomic dataen
dc.subjectatomic processesen
dc.subjectline: formationen
dc.subjectx-rays: generalen
dc.subjectx-ray-spectrumen
dc.subjectdielectronic satellite spectraen
dc.subjectlithium-like ionsen
dc.subjectr-matrix approachen
dc.subjectbe-like systemsen
dc.subjectisoelectronic sequenceen
dc.subjectfine-structureen
dc.subjectatomic dataen
dc.subjectxmm-newtonen
dc.subjectradiative transitionsen
dc.titleNitrogen K-Shell Photoabsorptionen
dc.typeArticle - Refereeden
dc.contributor.departmentPhysicsen
dc.identifier.urlhttp://iopscience.iop.org/0067-0049/185/2/477/en
dc.date.accessed2014-02-28en
dc.title.serialAstrophysical Journal Supplement Seriesen
dc.identifier.doihttps://doi.org/10.1088/0067-0049/185/2/477en


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