Four measures of the intracluster medium temperature and their relation toa cluster's dynamical state

Citation
Bf. Mathiesen et Ae. Evrard, Four measures of the intracluster medium temperature and their relation toa cluster's dynamical state, ASTROPHYS J, 546(1), 2001, pp. 100-116
Citations number
36
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
546
Issue
1
Year of publication
2001
Part
1
Pages
100 - 116
Database
ISI
SICI code
0004-637X(20010101)546:1<100:FMOTIM>2.0.ZU;2-2
Abstract
We employ an ensemble of 24 hydrodynamic cluster simulations to create spat ially and spectrally resolved images of quality comparable to Chandra's exp ected performance. Emission from simulation mass elements is represented us ing the XSPEC "MEKAL" program assuming 0.3 solar metallicity and the result ing spectra are fitted with a single-temperature model. Despite significant departures from isothermality in the cluster gas, single-temperature model s produce acceptable fits to 20,000 source photon spectra. The spectral fit temperature T-s is generally lower than the mass-weighted average temperat ure T-m due to the influence of soft line emission from cooler gas being ac creted as part of the hierarchical clustering process. The nature of this d eviation depends on the bandpass used for spectral fitting. In a Chandra-li ke bandpass of 0.5 to 9.5 keV we find a nearly uniform fractional bias of ( T-m - T-s)/T-s similar or equal to 20%, although smaller clusters sometimes demonstrate much greater deviations. If the minimum energy threshold is ra ised to 2 keV, however, the effect of line emission on the spectrum is grea tly decreased and T-s becomes a nearly unbiased estimator of for smaller cl usters. The fractional deviation in T-s relative to T-m is scale-dependent in this bandpass and follows the approximate relation (T-m - T-s)/T-s = 0.2 log(10) T-m. This results in an observed M-ICM-T-s relationship for the si mulations with slope of about 1.6, intermediate between the virial relation M proportional to T-m(3/2) and the observed relation M-ICM proportional to T-2. Tracking each cluster in the ensemble at 16 epochs in its evolutionar y history, we catalog merger events with mass ratios exceeding 10% in order to investigate the relationship between spectral temperature and proximity to a major merger event. Clusters that are very cool relative to the mean mass-temperature relationship lie preferentially close to a major merger, s uggesting a viable observational method to cull a subset of dynamically you ng clusters from the general population.