RS Canum Venaticorum stars

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RS Canum Venaticorum stars [¦är¦es ¦kan·ən və‚nad·ə¦kȯr·əm ‚stärz]

(astronomy)

A group of peculiar binary stars with orbital periods between 1 and 14 days, in which the cores of the H and K lines of singly ionized calcium display strong emission, and the hotter of the two stars is of spectral type F or G.

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