Oxygen recombination lines from Cas A knots (Docenko+, 2008)

Details Oxygen recombination lines from Cas A knots (Docenko+, 2008) Oxygen recombination lines from Cas A knots (Docenko+, 2008)

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34840755d&link_type=abstract

VizieR On-line Data Catalog: J/A+A/484/755. Originally published in: 2008A&A...484..755D

Physics

Atomic Physics

Supernova Remnants, Atomic Physics

Scientific paper

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).

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