Abundance gradients in cooling flow clusters: GINGA Large Area Counters and Einstein Solid State Spectrometer spectra of A496, A1795, A2142, and A2199

Details Abundance gradients in cooling flow clusters: GINGA Large Area Counters and Einstein Solid State Spectrometer spectra of A496, A1795, A2142, and A2199 Abundance gradients in cooling flow clusters: GINGA Large Area Counters and Einstein Solid State Spectrometer spectra of A496, A1795, A2142, and A2199

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...433..583w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 433, no. 2, p. 583-601

Astronomy and Astrophysics

Astrophysics

40

Abundance, Astronomical Models, Cooling Flows (Astrophysics), Galactic Clusters, Gradients, Metallicity, X Ray Astronomy, Computerized Simulation, Counters, Ginga Satellite, Heao 2, Spectrometers, X Ray Absorption, X Ray Spectra

Scientific paper

We analyze the Ginga Large Area Counters (LAC) and Einstein Solid State Spectrometer (SSS) spectra of four cooling flow clusters, A496, A1795, A2142, and A2199, each of which shows firm evidence of a relatively cool component. The inclusion of such cool spectral components in joint fits of SSS and LAC data leads to somewhat higher global temperatures than are derived from the high-energy LAC data alone. We find little evidence of cool emission outside the SSS field of view. Metal abundances appear to be centrally enhanced in all four clusters, with varying degrees of model dependence and statistical significance: the evidence is statistically strongest for A496 and A2142, somewhat weaker for A2199 and weakest for A1795. We also explore the model dependence in the amount of cold, X-ray-absorbing matter discovered in these clusters by White et al.

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