HEAD 2003 Meeting
Session 13. Galaxy Clusters III
Poster, Sunday-Wednesday, March 23, 2003, Duration of Meeting

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[13.05] A massive warm baryonic halo in the Coma cluster

M. Bonamente (UAH), M.K. Joy (NASA/MSFC), R. Lieu (UAH)

Several deep PSPC observations of the Coma cluster reveal a very large-scale halo of soft X-ray emission, substantially in excess of the well known radiation from the hot intra-cluster medium. The excess emission, previously reported in the central region of the cluster using lower-sensitivity EUVE and ROSAT data, is now evident out to a radius of 2.6 Mpc, demonstrating that the soft excess radiation from clusters is a phenomenon of cosmological significance. The X-ray spectrum at these large radii cannot be modeled non-thermally, but is consistent with the original scenario of thermal emission from warm gas at ~ 106 K. The mass of the warm gas is on par with that of the hot X-ray emitting plasma, and significantly more massive if the warm gas resides in low-density filamentary structures. Thus the data lend vital support to current theories of cosmic evolution, which predict that at low redshift ~ 30-40 % of the baryons reside in warm filaments converging at clusters of galaxies.

The author(s) of this abstract have provided an email address for comments about the abstract: bonamem@email.uah.edu

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Bulletin of the American Astronomical Society, 35#2
© 2003. The American Astronomical Soceity.