Mike Garcia and colleagues use Chandra and HST to find a possible 3 x 10^35 erg/s source coincident with the central black hole in M31.
Fujita et al. use hydro simulations to predict high resolution X-ray spectra observed with Astro-E2.
Asai et al. do MHD simulations of a galaxy moving through the ICM and show that a magnetized medium is required to produce the cometary tail seen in Chandra observations of A2125.
Nicastro et al. estimate the mass density of the WHIM using results from X-ray absorption spectroscopy and show that it is consistent with the predicted value.
Keywords: papers, black holes, clusters, WHIM
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