Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...384l..19c&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 384, Jan. 1, 1992, p. L19-L23.
Astronomy and Astrophysics
Astronomy
16
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.
Clayton Geoffrey C.
Drilling John S.
Judge Philip G.
Stanford Spencer A.
Whitney Barbara A.
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