Fig. 1 from Tomographic Separation of Composite Spectra. IX. The Massive Close Binary HD 115071

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Tomographic Separation of Composite Spectra. IX. The Massive Close Binary HD 115071

Authors: Laura R. Penny, Douglas R. Gies, John H. Wise, D. J. Stickland, and C. Lloyd

Penny et al. 2002 The Astrophysical Journal 575 1050.

Provider: AAS Journals

Caption: Fig. 1.

Radial velocity measurements (filled circles: primary; open circles: secondary) and orbital solution (solid lines) plotted against orbital phase. Phase zero corresponds to the time of primary maximum radial velocity. The two plus marks show the IUE measurements that were not used in the solution.

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