Fig. 1 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. 1.

Residuals of our transformation vs. color, expressed in the sense of observed minus fitted magnitude. As is typical for this passband, the residuals in U are comparatively large. However, we see no systematic increase in the size of residuals in any of our filters as colors become bluer.

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