Late-type Ca II emission-line stars in the Southern Hemisphere
The results of a photometric and spectroscopic study of twenty-three late-type southern stars with strong Ca II H and K emission are presented. The presence of photometric variability, with similar properties to the photometric wave phenomenon seen in the RS Canum Venaticorum binaries, is noted in...
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| Language: | en |
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University of Canterbury.
2013
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| Online Access: | http://hdl.handle.net/10092/8057 |