On the 1893 absorption-line spectrum of Eta Carinae

Details On the 1893 absorption-line spectrum of Eta Carinae On the 1893 absorption-line spectrum of Eta Carinae

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..578b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 688, p. 578.

Astronomy and Astrophysics

Astronomy

2

Absorption Spectra, Line Spectra, Stellar Spectra, Variable Stars, Abundance, Carbon

Scientific paper

It is suggested that several features present in the 1893
absorption-line spectrum of Eta Carinae may be due to high-excitation
lines of neutral carbon not seen in the spectra of stars of normal
chemical composition. This perhaps implies a relationship of this unique
southern variable to the stars of the R Coronae Borealis type.

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