Image Details
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.
© 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.