Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...412..489k&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 412, no. 2, p. 489-503.
Astronomy and Astrophysics
Astronomy
25
Cosmic Gases, Galactic Clusters, Metallicity, Spaceborne Astronomy, Spartan Satellites, X Ray Astronomy, Intergalactic Media, Iron
Scientific paper
The Spartan 1 instrument has resolved the spatial and spectral distribution of the 1-10 keV X-ray emission from the Perseus cluster in a region extending 50 arcmin from the center. The data were fitted with a spherically symmetric three-dimensional model which included separate components for the cooling flow, the extended cluster emission, and a possible point source located at NGC 1275. A careful study has been made of the abundance distribution of iron as a function of radius. We confirm the existence of a gradient where the best-fit central abundance is 0.77 + 0.30 of - 0.38 times the solar value and the linear gradient is -1.10 + 0.89 or - 2.24 per Mpc (90 percent confidence for a single interesting parameter in both cases). Joint 90 percent confidence limits to the abundance parameters have been established, and the resulting limits to the abundance distribution have been applied to theoretical models of cluster structure and evolution. We find that our results are consistent with a gas-removal mechanism with enhanced efficiency at the cluster center such as ram-pressure stripping or thermal exaporation. Our results are also in agreement with cluster evolution models in which the initial density of primordial gas in the cluster formation region is high (not less than 10 exp 28 g/cu cm).
Cruddace Ray G.
Fenimore Edward E.
Fritz Georg
Kowalski Piotr M.
Snyder W. A.
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