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The Open Cluster NGC 2516. I. Optical Photometry

  • Authors: Hwankyung Sung, Michael S. Bessell, Bo-Won Lee, and Sang-Gak Lee

Sung et al. 2002 The Astronomical Journal 123 290.

  • Provider: AAS Journals

Caption: Fig. 5.

Color excesses. (a) δ(UB) = (UB)0−(UB)ZAMS at a given (VI)0. (b) δ(BV) = (BV)0−(BV)ZAMS at a given (VI)0. The crosses represent X‐ray emission stars. The dotted lines represent the color excess difference between the Z = 0.019 and Z = 0.008 models from Girardi et al. (2000). The size of the circles are proportional to the number of normal stars in the color bin [Δ(VI) = 0.2 mag]. The error bars indicate the standard deviation of the stars in the bin. The thick solid line represents the correction applied to BV in the calculation of distance modulus in the V vs. BV diagram.

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