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Abstract:
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We present a Chandra, Suzaku and Rosat study of the hot Intra Group Medium (IGrM) of the
relaxed fossil group/ poor cluster RXJ 1159+5531. This group exhibits an advantageous combination
of flat surface brightness profile, high luminosity and optimal distance, allowing the gas to be detected
out to the virial radius (Rvir≡ R108 =1100 kpc) in a single Suzaku pointing, while the complementary
Chandra data reveal a round morphology and relaxed IGrMimage down to kpc scales. We measure the
IGrM entropy profile over ∼3 orders of magnitude in radius, including 3 data bins beyond ∼ 0.5R200
that have good azimuthal coverage (>30%). We find no evidence that the profile flattens at large
scales (>R500), and when corrected for the enclosed gas fraction, the entropy profile is very close to
the predictions from self-similar structure formation simulations, as seen in massive clusters. Within
Rvir, we measure a baryon fraction of 0.17 ± 0.02, consistent with the Cosmological value. These
results are in sharp contrast to the gas behaviour at large scales recently reported in the Virgo and
Perseus clusters, and indicate that substantial gas clumping cannot be ubiquitous near Rvir, at least
in highly evolved (fossil) groups. |