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On X‐Ray Variability in Active Binary Stars

  • Authors: Vinay Kashyap and Jeremy J. Drake

Kashyap & Drake 1999 The Astrophysical Journal 524 988.

  • Provider: AAS Journals

Caption: Fig. 1.

Scatter plot of count rates observed at different epochs: RASSBSC vs. Einstein. The Einstein count rates have been uniformly multiplied by a factor of 3.7 as derived by a straight‐line fit to the Einstein‐RASSBSC data set. The size of the 1 σ errors on the rates is indicated by the horizontal and vertical lines at each point. The solid inclined line represents the line of equality and the dotted lines flanking it represent variations of factors of 2.

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