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E. Rasia, G. Tormen and L. Moscardini, “A Dynamical Model for the Distribution of Dark Matter and Gas in Galaxy Clusters,” MNRAS, Vol. 351, No. 1, 2004, pp. 237-252. doi:10.1111/j.1365-2966.2004.07775.x

has been cited by the following article:

• TITLE: The Cherenkov Radiation in the Galaxy’s Halo of Dark Matter

  AUTHORS: Leonid M. Chechin

  KEYWORDS: Dark Matter Profile; The Cherenkov Radiation

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.3 No.3, September 3, 2013

  ABSTRACT: The effect of light refraction in a galaxy’s halo of dark matter, described by profiles of Navarro-Frenk-White and Burkert, was considered. Powers of the Cherenkov radiation for the refractive indexes of gravitational fields with these profiles were calculated. It was shown that correspondent radiation temperature in the X-rays diapason have the magnitude about T~10-6K . It was also marked that its detection may be the criteria on choosing the preferable dark matter density distribution in a galaxy.