The long-period Galactic Cepheid RS Puppis - III. A geometric distance from HST polarimetric imaging of its light echoes

P. Kervella; H. E. Bond; M. Cracraft; L. Szabados; J. Breitfelder; A. Mérand; W. B. Sparks; A. Gallenne; D. Bersier; P. Fouqué; R. I. Anderson

doi:10.1051/0004-6361/201424395

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Volume 572 (December 2014)

A&A, 572 (2014) A7

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Fig. 7

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Median p_L values observed in the nebula of RS Pup in 1% bins as a function of the percentile of highest values. The attached vertical segments show the full range of values of p_L in each bin. The orange segment on the vertical axis shows the adopted uncertainty range for p_max = 51.5% ± 2.0%.

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