Fig. 3 from Tomographic Separation of Composite Spectra. IX. The Massive Close Binary HD 115071

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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. 3.

Hipparcos light curve plotted against spectroscopic orbital phase. The solid line shows the predicted curve for a secondary Roche‐filling model with ﹩i=48\fdg 7﹩, while the dashed line represents the prediction for an underfilling model with ﹩i=60^{\circ }﹩.

Other Images in This Article

Copyright and Terms & Conditions