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Multiwavelength Optical Observations of Two Chromospherically Active Binary Systems: V789 Mon and GZ Leo

  • Authors: M. C. Gálvez, D. Montes, M. J. Fernández-Figueroa, E. De-Castro, and M. Cornide

GÁLVEZ et al. 2009 The Astronomical Journal 137 3965.

  • Provider: AAS Journals

Caption: Figure 1.

Radial velocity data and fit vs. the orbital phase. Solid symbols represent the primary and open symbols represent the secondary. V789 Mon (2RE J0725 − 002) on the left (squares data from Jeffries et al. 1995 and circles data from our observations) and GZ Leo (2RE J1101+223) on the right (squares data from Jeffries et al. 1995, triangles from Fekel & Henry 2000, rhombus from Strassmeier et al. 2000, circles from our McDonald98 observing run and stars from our FOCES02 observing run). The solid curves represent a minimum χ 2 fit orbit solution as described in the text.

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