Direct X‐ray spectral deprojection of galaxy clusters

@article{Russell2008DirectXS,
  title={Direct X‐ray spectral deprojection of galaxy clusters},
  author={H. Russell and J. Sanders and A. Fabian},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2008},
  volume={390},
  pages={1207-1216}
}
  • H. Russell, J. Sanders, A. Fabian
  • Published 2008
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • Temperature, density and abundance profiles of the hot intracluster medium (ICM) are important diagnostics of the complex interactions of gravitational and feedback processes in the cores of galaxy clusters. Deprojection of X-ray data by methods such as projct, which are model dependent, can produce large and unphysical oscillating temperature profiles. Here, we validate a deprojection routine, Direct Spectral Deprojection (dsdeproj), showing that it solves some of the issues inherent to model… CONTINUE READING

    Figures from this paper.

    Probing the Outskirts of the Early-Stage Galaxy Cluster Merger A1750
    • 18
    • PDF
    Cooling in the X-ray halo of the rotating, massive early-type galaxy NGC 7049
    • 7
    • PDF
    Inside the Bondi radius of M87
    • 60
    • PDF

    References

    Publications referenced by this paper.
    SHOWING 1-10 OF 45 REFERENCES
    Spatially resolved X-ray spectroscopy of cooling clusters of galaxies
    • 156
    • PDF
    The galaxy cluster Abell 3581 as seen by Chandra
    • 23
    • PDF
    X-ray Spectroscopy of Cooling Clusters
    • 353
    • PDF
    Chandra imaging of the complex X-ray core of the Perseus cluster
    • 441
    • PDF
    The Cluster-Scale AGN Outburst in Hydra A
    • 192
    • PDF
    Reflections of Active Galactic Nucleus Outbursts in the Gaseous Atmosphere of M87
    • 215
    • PDF
    Heating Hot Atmospheres with Active Galactic Nuclei
    • 823
    • PDF