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Home › Image Galleries › Peter Mendygral › RE Observations ›

2 keV Observation of RE at 157 Myr - Beta Divided

Submitted by peter on Wed, 12/17/2008 - 13:49
  • RE Observations

Introduction
This is an X-ray observation of the RE simulation at 157 Myr divided by a best fit double β-profile to emphasize the cavities. We have included thermal Bremsstrahlung and inverse Compton emission from 1.5 to 2.5 keV here.

2 keV Observation of RE at 157 Myr - Beta Divided
‹ 40 keV Observation of RE at 157 Myr up 10 keV Observation of RE at 157 Myr - Beta Divided ›
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  • WOMBAT - Astrophysical Fluid Code
  • Multidimensional DSA
  • Stellar Winds
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    • AGN in Dynamic Clusters
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      • Relic (RE) Simulation
      • Synthetic Observations of Radio Jets in Cluster Environments
        • RE Observations
          • 300 MHz Observation of RE at 157 Myr
          • 1.4 GHz Observation of RE at 157 Myr
          • 2 keV Observation of RE at 157 Myr
          • 10 keV Observation of RE at 157 Myr
          • 25 keV Observation of RE at 157 Myr
          • 40 keV Observation of RE at 157 Myr
          • 2 keV Observation of RE at 157 Myr - Beta Divided
          • 10 keV Observation of RE at 157 Myr - Beta Divided
        • I13 Observations
      • Narrow Angle Tail Simulation
    • Dual (Orbiting) AGN
  • Buoyant Bubbles in Galaxy Clusters
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University of Minnesota :: Minnesota Institute of Astrophysics
Contact :: Tom Jones :: twj@msi.umn.edu