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Home › Image Galleries › Peter Mendygral › I13 Observations ›

25 keV Observation of I13 at 171 Myr

Submitted by peter on Thu, 12/18/2008 - 13:49
  • I13 Observations

Introduction
This is an X-ray observation of the I13 simulation at 171 Myr. We have included thermal Bremsstrahlung and inverse Compton emission from 24.5 to 25.5 keV here. To compute a realistic flux the grid was placed at 240 Mpc. The units across the bottom are 10-23 erg s-1 cm-2 arcsec-2.

At higher energies we have started to pick up significant inverse Compton emission from a within the jet material. An interesting aspect of this emission is that most of it is coming from a sheath that surrounds the cavity. This region is real mixing between ICM and AGN plasma.

25 keV Observation of I13 at 171 Myr
‹ 10 keV Observation of I13 at 171 Myr up 40 keV Observation of I13 at 171 Myr ›
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  • WOMBAT - Astrophysical Fluid Code
  • Multidimensional DSA
  • Stellar Winds
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  • AGN Jets in Galaxy Clusters
    • AGN in Dynamic Clusters
    • AGN in Idealized Clusters
      • Relic (RE) Simulation
      • Synthetic Observations of Radio Jets in Cluster Environments
        • RE Observations
        • I13 Observations
          • 300 MHz Observation of I13 at 171 Myr
          • 1.4 GHz Observation of I13 at 171 Myr
          • 2 keV Observation of I13 at 171 Myr
          • 10 keV Observation of I13 at 171 Myr
          • 25 keV Observation of I13 at 171 Myr
          • 40 keV Observation of I13 at 171 Myr
          • 2 keV Observation of RE at 171 Myr - Beta Divided
          • 10 keV Observation of I13 at 171 Myr - Beta Divided
          • 2 keV + 1.4 GHz Observations of I13 at 171 Myr
      • Narrow Angle Tail Simulation
    • Dual (Orbiting) AGN
  • Buoyant Bubbles in Galaxy Clusters
  • Galactic Superbubbles
  • MHD Turbulence

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University of Minnesota :: Minnesota Institute of Astrophysics
Contact :: Tom Jones :: twj@msi.umn.edu