NSV 6708 - Hydrogen in an R Coronae Borealis star

Details NSV 6708 - Hydrogen in an R Coronae Borealis star NSV 6708 - Hydrogen in an R Coronae Borealis star

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.238p...1k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 238, May 1, 1989, p. 1P-6P.

Astronomy and Astrophysics

Astronomy

29

H Lines, Stellar Composition, Stellar Spectrophotometry, Variable Stars, Balmer Series, Hydrogen, Ubv Spectra

Scientific paper

The photometric behavior and spectroscopic appearance of NSV 6708 are typical of the R Coronae Borealis class of variable star, except that Balmer series hydrogen lines are clearly present in the spectrum. The limited observations available indicate that NSV 6708 is very active in producing 'deep' or obscurational minima and it is suggested that the star may be currently ejecting its 'hydrogen-rich' outer layers.

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