Fig. 6 from The Distance to the Large Magellanic Cloud via the Eclipsing Binary HV 2274

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The Distance to the Large Magellanic Cloud via the Eclipsing Binary HV 2274

Authors: Cailin A. Nelson, Kem H. Cook, Piotr Popowski, and David R. Alves

Nelson et al. 2000 The Astronomical Journal 119 1205.

Provider: AAS Journals

Caption: Fig. 6.

B−V vs. Q plot for HV 2274 and nearby O/B stars. The line is a fiducial of unreddened Galactic O/B stars. The reddening, E(B−V), of a star is measured as its vertical displacement from the unreddened line.

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