Image Details
Caption: Fig. 3.
Plot of the long‐term variations in the Hα line profile. The phase shown immediately above the left wing of each line profile was calculated using Harmanec's (1984) ephemeris and corresponds to the mean HJD given just above the right wing of each line profile. The spectra are separated by 100% of the continuum for visual clarity.
© 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.