VizieR Online Data Catalog: New FeII energy levels from stellar spectra (Castelli+, 2010)
Abstract
FeII lines in the 3800-8000Å region, produced by transitions to the FeII subconfigurations (3P)4f, (3H)4f, (3F)4f, and (3G)4f are given in Tables 6, 7, 8, and 9, respectively. Only lines with loggf>=-1.5 are listed. Most of these lines can be observed in the UVES spectrum of HR 6000 and have allowed us to identify more than 50% of the previously unidentified lines (Castelli & Hubrig, 2007A&A...475.1041C).
(4 data files).- Publication:
-
VizieR Online Data Catalog
- Pub Date:
- July 2010
- DOI:
- 10.26093/cds/vizier.35200057
- Bibcode:
- 2010yCat..35200057C
- Keywords:
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- Atomic physics;
- Line Profiles;
- Models: atmosphere;
- Spectroscopy;
- Stars: peculiar