Evidence of Tidal Effects in Some Pulsating Stars. I CC Andromedae and Sigma Scorpii
Analyses of the light variation of the 6 Scuti star CC Andromedae and of the radial velocity variation of the ß Canis Majoris star 6 Scorpii, a single -line spectroscopic binary, indicate that the long period modulations exhibited are caused by tidal deformations induced in the hydrogen and /or...
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| Language: | en_US |
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Steward Observatory, The University of Arizona (Tucson, Arizona)
1966
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| Online Access: | http://hdl.handle.net/10150/623810 http://arizona.openrepository.com/arizona/handle/10150/623810 |