VizieR Online Data Catalog: Oxygen recombination lines from Cas A knots (Docenko+, 2008)
Abstract
Tables contain wavelengths and intensities or emissivities of the fine structure components of the O, Si and S ion optical and near-infrared recombination lines (RLs) in the (nlK) -> (n'l'K') resolution.
Emissivities and wavelengths are given for O II-VI, Si II-III and S II-V ion {alpha}-, {beta}- and {gamma}-line components in the wavelength range between 0.3 and 5 micron and temperature range between 103 and 105K. Only low-density emissivity values are included in tables and only transitions onto levels with nl>=5 are considered. Intensities and wavelengths are given for O II-VI ion {alpha}-, {beta}- and {gamma}-line components in the same wavelength range, as computed based on the Sutherland & Dopita (1995ApJ...439..381S) model of the oxygen-rich plasma emission in supernova remnants applied to Cassiopeia A fast-moving knots. (19 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- March 2008
- DOI:
- 10.26093/cds/vizier.34840755
- Bibcode:
- 2008yCat..34840755D
- Keywords:
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- Supernova remnants;
- Atomic physics