Fig. 2 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. 2.

Comparison of the reconstructed MSO spectra (above) and CASLEO spectra (below) of the primary and the secondary with spectra of the same classifications as Walborn & Fitzpatrick (1990). All the spectra were Gaussian smoothed to a nominal resolution of 1.2 Å FWHM for consistent line broadening.

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