Image Details
Caption: Fig. 1.
Properties of long‐period variables, from AAVSO observations analyzed with the CLEANest algorithm. The abscissa is amplitude A in visual magnitude, and the ordinate is the rms scatter in the amplitude. Plus signs and diamonds show stars that have been classified as Mira variables and SR variables, respectively. Adapted from Mattei et al. (1997).
© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.