Image Details
Caption: Fig. 3.
The rms scatter in amplitude vs. amplitude for the low‐amplitude sample of AAVSO stars (see also Fig. 1). Plus signs and diamonds show stars that have been classified as Mira variables and SR variables, respectively. The solid line shows the theoretical relation for stochastically excited oscillators, from eq. (2).
© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.