Presence of MG II emission in R Coronae Borealis at maximum light

Details Presence of MG II emission in R Coronae Borealis at maximum light Presence of MG II emission in R Coronae Borealis at maximum light

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.195p..71k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 195, June 1981, p. 71P-74P.

Astronomy and Astrophysics

Astronomy

14

Carbon Stars, Emission Spectra, Magnesium, R Coronae Borealis Stars, Stellar Spectra, Variable Stars, Chromosphere, Iue, Metallic Stars, Spaceborne Astronomy

Scientific paper

The high dipersion spectrum of R CrB in the long wavelength obtained
near its maximum with the International Ultraviolet Explorer shows the
presence of chromospheric Mg II emission. For comparison the spectrum of
Gamma Cyg was obtained immediately afterwards. The Mg II emission width
of R CrB is found to be the same as that of Gamma Cyg.

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