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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. 9.

Luminosity function and mass function of NGC 2516. The open and filled circles are the calculated LF with bin size ΔMV = 1 mag but shifted by 0.5 mag to smooth out the binning effect. The transformation from LF to MF is described in the text. The thick solid line represents the MF slope for log m ≥ −0.1, while the thin line denotes the initial mass function of the solar neighborhood from Lee & Sung (1995) normalized at log m = 0.5 to −0.1.

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