A Model for the Extended X-Ray Source Surrounding M87

Details A Model for the Extended X-Ray Source Surrounding M87 A Model for the Extended X-Ray Source Surrounding M87

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pthph..65..369t&link_type=abstract

Progress of Theoretical Physics, Vol. 65, No. 1, pp. 369-373

Physics

23

Scientific paper

We show that the properties of the X-ray source surrounding M87 are well
explained by thermal emission from the gas in hydrostatic equilibrium in
the gravitational potential well of the massive halo of M87, where
radiative cooling is balanced by conductive heat flux from the ambient,
hot intracluster gas.

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