Fe II emission lines of RR Tel

DOI

Files table1.dat and table2.dat contain the permitted and forbidden Fe II emission lines respectively which have been selected from the optical spectrum of RR Tel between 3180 and 9455{AA}. The spectrum was observed by Crawford et al. (1999, Cat. ) whose corrected line fluxes and velocity widths we took for further analysis in this work. In the tables there are also values characteristic for the corresponding multiplets and lines such as multiplet numbers, term designations, level excitation potentials and quantum numbers J. The log functions of gf's, line fluxes and wavelengths are relevant for the SAC curves.

Identifier
DOI http://doi.org/10.26093/cds/vizier.33810507
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/381/507
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/381/507
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/381/507
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/381/507
Provenance
Creator Kotnik-Karuza D.; Friedjung M.; Selvelli P.L.
Publisher CDS
Publication Year 2002
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy