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A New Cepheid Distance Measurement and Method for NGC 6822

  • Authors: Jeffrey A. Rich, S. E. Persson, Wendy L. Freedman, Barry F. Madore, Andrew J. Monson, Victoria Scowcroft, and Mark Seibert

Rich et al. 2014 The Astrophysical Journal 794 107.

  • Provider: AAS Journals

Caption: Figure 4.

First method for calculating a true distance modulus, μo and E(BV). Data points correspond to the distance modulus from each band plotted as a function of inverse wavelength, λ−1. A reddening-law fit to the moduli (excluding 4.5 μm) is plotted as the solid line. The Cardelli et al. (1989) reddening law was used with a fixed Rv = 3.1 and E(BV) and μo allowed to vary. The resulting fit provides an extinction-corrected distance modulus of 23.38 ± 0.05 mag and E(BV) = 0.36 ± 0.09.

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