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The Spectral Components of SS 433

  • Authors: D. R. Gies, M. V. McSwain, R. L. Riddle, Z. Wang, P. J. Wiita, and D. W. Wingert

Gies et al. 2002 The Astrophysical Journal 566 1069.

  • Provider: AAS Journals

Caption: Fig. 7.

Individual Hα stationary profiles from our final run plotted in the same format as Fig. 6. Here the dashed line shows the fitted radial velocity curve for the Hα− jet, while the dash–triple‐dotted line shows the same for jet features of He I ﹩\lambda 6678﹩. The dash–single‐dotted line shows the radial velocity curve of the opposite red jet for He I ﹩\lambda 5876﹩. No He I jet components are readily visible at their expected positions. The nearly vertical dotted line traces the outward motion of a redshifted emission bump.

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