The unusual ultraviolet chromospheric spectrum of the R Coronae Borealis star, V854 Centauri (NSV 6708), at minimum light

Astronomy and Astrophysics – Astronomy

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Chromosphere, R Coronae Borealis Stars, Stellar Coronas, Stellar Spectra, Ultraviolet Spectra, Iue, Line Spectra, Spectrum Analysis, Ultraviolet Astronomy

Scientific paper

Results are presented of IUE observations of a decline of the recently discovered R CrB star, V854 Cen. These observations are of particular interest because they include spectra taken at 7 mag below maximum light. The 'chromospheric' emission spectra show striking differences from UV spectra of other R CrB stars in decline. Strong emission appears in several lines not normally seen in R CrB emission-line spectra, in particular at semiforbidden C II 2326, Mg I 2852, and C I 2965, 2967. Spectral evolution similar to that seen in visible spectra of R CrB stars is clearly seen in the UV. It is argued that the differences between V854 Cen and other R CrB stars are related to known abundance differences or to different temperature and density conditions in the emission-line regions of the various R CrB stars. The emission may also be significantly affected by the presence of dust in or near the emitting region.

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