Fig. 3 from ROSAT and BeppoSAX Evidence of Soft X‐Ray Excess Emission in the Shapley Supercluster: A3571, A3558, A3560, and A3562

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

ROSAT and BeppoSAX Evidence of Soft X‐Ray Excess Emission in the Shapley Supercluster: A3571, A3558, A3560, and A3562

Authors: Massimiliano Bonamente, Richard Lieu, Jukka Nevalainen, and Jelle S. Kaastra

Bonamente et al. 2001 The Astrophysical Journal Letters 552 L7.

Provider: AAS Journals

Caption: Fig. 3.

Same as Fig. 2, but for the fractional R34 band excess ﹩\zeta =( p_{34}-q_{34}) / q_{34}﹩ where ﹩p_{34}﹩ is the observed R34 band flux and ﹩q_{34}﹩ is the expected R34 band flux from the hot ICM.

Other Images in This Article

Copyright and Terms & Conditions