Anomalous ratios of emission line intensities in the spectrum of RW Aurigae

Physics

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Auriga Constellation, Emission Spectra, Line Spectra, Stellar Spectra, Anomalies, Fluorescence, Radiant Flux Density, Stellar Radiation

Scientific paper

The intensity ratios of neutral iron lines in the spectrum of RW Aur are
studied. No fluorescent process is found in the 430.7-nm Fe I (42) line.
The quantitative characteristics of the anomalous strengthening of the
406.3 and 413.2 nm Fe I (43) lines and the weakening of the H Ca II line
are obtained.

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