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2004MNRAS.349.1240K - Mon. Not. R. Astron. Soc., 349, 1240-1250 (2004/April-3)
An old galaxy group: Chandra X-ray observations of the nearby fossil group NGC 6482.
KHOSROSHAHI H.G., JONES L.R. and PONMAN T.J.
Abstract (from CDS):
Although the cooling time within 0.1r200is less than a Hubble time, no decrease in central temperature is detected. The entropy of the system lies toward the low side of the distribution seen in poor groups and drops all the way into the centre of the system, reaching very low values. No isentropic core, such as those predicted in simple pre-heating models, is present. Given the lack of any central temperature drop in the system, it seems unlikely that radiative cooling can be invoked to explain this low central entropy. The lack of any signature of central cooling is especially striking in a system that appears to be old and relaxed, and to have a central cooling time ≤108 yr. We find that the centrally peaked temperature profile is consistent with a steady-state cooling-flow solution with an accretion rate of 2 M☉/yr, given the large P dV work arising from the cuspy mass profile. However, solutions involving distributed or non-steady heating cannot be ruled out.
Abstract Copyright: 2004 RAS
Journal keyword(s): galaxies: clusters: general - galaxies: elliptical and lenticular, cD - galaxies: haloes - intergalactic medium - X-rays: galaxies - X-rays: galaxies: clusters
Simbad objects: 11
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