Fig. 2 from Radial Velocity Studies of Close Binary Stars. V.

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Radial Velocity Studies of Close Binary Stars. V.

Authors: Slavek M. Rucinski, Wenxian Lu, Stefan W. Mochnacki, Waldemar Ogłoza, and Greg Stachowski

Rucinski et al. 2001 The Astronomical Journal 122 1974.

Provider: AAS Journals

Caption: Fig. 2.

Same as for Fig. 1, but with the radial velocity orbits for the systems FN Cam, V776 Cas, SX Crv, and V351 Peg. Only V351 Peg is a W‐type system, the others are A‐type systems. SX Crv is a new record holder with a mass ratio of only ﹩q=0.066\pm 0.003﹩.

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