Figure 4 from No Excess of RR Lyrae Stars in the Canis Major Overdensity

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No Excess of RR Lyrae Stars in the Canis Major Overdensity

Authors: Cecilia Mateu, A. Katherina Vivas, Robert Zinn, Lissa R. Miller, and Carlos Abad

MATEU et al. 2009 The Astronomical Journal 137 4412.

Caption: Figure 4.

Light curves of the identified W UMa eclipsing contact binaries. Symbols are as in Figure 3. The solid lines show the best-fitting template.