The X-ray properties of the radio galaxy B2 1122+39.

Details The X-ray properties of the radio galaxy B2 1122+39. The X-ray properties of the radio galaxy B2 1122+39.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..475m&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 475 - 476

Astronomy and Astrophysics

Astrophysics

Radio Galaxies: X Rays, Radio Galaxies: Radio Radiation, Radio Galaxies: Morphology

Scientific paper

The radiogalaxy B2 1122+39, associated with two radio jets, has been observed with the PSPC and HRI instruments of ROSAT. An extended X-ray emission from a halo of hot gas (kT ≡ 0.5 keV) surrounding the galaxy has been detected, with brightness distribution consistent with an hydrostatic β model. From the comparison of the X-ray data with radio observations the authors find that the pressure is lower in the jet than in the external gas. The standard equipartition assumptions may not be valid.

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