Now showing items 1-2 of 2

    • Hundred thousand degree gas in the virgo cluster of galaxies. 

      Sparks, W.B.; Pringle, J. E.; Carswell, R. F.; Donahue, M.; Martin, R.; Voit, M.; Cracraft, M.; Manset, N.; Hough, J. H. (2012-05-01)
      The physical relationship between low-excitation gas filaments at similar to 10(4) K, seen in optical line emission, and diffuse X-ray emitting coronal gas at similar to 10(7) K in the centers of many galaxy clusters is ...
    • Polarization Diagnostics for Cool Core Cluster Emission Lines 

      Sparks, W.B.; Pringle, J. E.; Carswell, R. F.; Voit, G.M.; Donahue, M.; Cracraft, M.; Meyer, E.T.; Hough, J.H.; Manset, N. (2014-01-01)
      The nature of the interaction between low-excitation gas filaments at ~104 K, seen in optical line emission, and diffuse X-ray emitting coronal gas at ~107 K in the centers of galaxy clusters remains a puzzle. The presence ...