Image Details

Choose export citation format:

Large resolution
Export to PDF

X‐Ray Time Variability Across the Atoll Source States of 4U 1636−53

  • Authors: D. Altamirano, M. van der Klis, M. Méndez, P. G. Jonker, M. Klein-Wolt, and W. H. G. Lewin

Altamirano et al. 2008 The Astrophysical Journal 685 436.

  • Provider: AAS Journals

Caption: Fig. 11.

Fractional rms amplitude of all components (except ﹩L_{\mathrm{LF}\,}﹩) vs. ﹩\nu _{u}﹩. The symbols are labeled in the top right plot. The data for 4U 1728−34, 4U 1608−52, and 4U 0614+09 were taken from van Straaten et al. (2005). Note that for ﹩L_{\mathrm{hHz}\,}﹩ and ﹩L_{h}﹩ of 4U 1608−52, the three triangles with vertical error bars which intersect the abscissa represent 95% confidence upper limits (see van Straaten et al. [2003] for a discussion). Also note that we exclude the three points in the rms vs. ﹩\nu _{u}﹩ plot which were identified as Lℓow by van Straaten et al. (2003).

Other Images in This Article

Show More

Copyright and Terms & Conditions