Now showing items 1-5 of 5

    • THE ACCRETION DISK WIND IN THE BLACK HOLE GRS 1915+105 

      Miller, JM; Raymond, J; Fabian, Andrew Christopher; Gallo, E; Kaastra, J; Kallman, T; King, AL et al. (2016-04-10)
    • DISK–WIND CONNECTION DURING THE HEARTBEATS OF GRS 1915+105 

      Zoghbi, A; Miller, JM; King, AL; Miller, MC; Proga, D; Kallman, T; Fabian, Andrew Christopher et al. (IOP Publishing, 2016-12-20)
      Disk and wind signatures are seen in the soft state of Galactic black holes, while the jet is seen in the hard state. Here we study the disk–wind connection in the ρ class of variability in GRS 1915+105 using a joint ...
    • POWERFUL, ROTATING DISK WINDS from STELLAR-MASS BLACK HOLES 

      Miller, JM; Fabian, Andrew Christopher; Kaastra, J; Kallman, T; King, AL; Proga, D; Raymond, J et al. (2015-12-01)
    • The quiescent intracluster medium in the core of the Perseus cluster 

      Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Anabuki, N; Angelini, L; Arnaud, K et al. (Nature Publishing Group, 2016-07-06)
      Clusters of galaxies are the most massive gravitationally bound objects in the Universe and are still forming. They are thus important probes of cosmological parameters and many astrophysical processes. However, knowledge ...
    • Solar abundance ratios of the iron-peak elements in the Perseus cluster 

      Aharonian, F; Akamatsu, H; Akimoto, F; Allen, SW; Angelini, L; Audard, M; Awaki, H et al. (2017-11-23)
      The metal abundance of the hot plasma that permeates galaxy clusters represents the accumulation of heavy elements produced by billions of supernovae. Therefore, X-ray spectroscopy of the intracluster medium provides an ...