The impact of mergers on relaxed X-ray clusters - II. Effects on global X-ray and Sunyaev-Zel'dovich properties and their scaling relations

被引:108
作者
Poole, Gregory B.
Babul, Arif
McCarthy, Ian G.
Fardal, Mark A.
Bildfell, C. J.
Quinn, Thomas
Mahdavi, Andisheh
机构
[1] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 1A1, Canada
[2] Univ Durham, Dept Phys, Durham DH1 3LE, England
[3] Univ Durham, Dept Astron, Amherst, MA 01003 USA
[4] Univ Durham, Dept Astron, Seattle, WA 98195 USA
关键词
galaxies : clusters : general; intergalactic medium; cosmology : theory; X-rays : general; GALAXY CLUSTERS; INTRACLUSTER MEDIUM; COOLING FLOWS; XMM-NEWTON; MASS; TEMPERATURE; EVOLUTION; ENTROPY; CHANDRA; LUMINOSITY;
D O I
10.1111/j.1365-2966.2007.12107.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use the suite of simulations presented by Poole et al. to examine global X-ray and Sunyaev-Zel'dovich (SZ) observables for systems of merging relaxed X-ray clusters. The time evolution of our merging systems' X-ray luminosities, temperatures, total mass measures, SZ central Compton parameters and integrated SZ fluxes are presented and the resulting impact on their scaling relations examined. In all cases, and for all parameters, we observe a common time evolution: two rapid transient increases during first and second pericentric passage, with interceding values near or below their initial levels. This is in good qualitative agreement with previous idealized merger simulations, although we find several important differences related to the inclusion of radiative cooling in our simulations. These trends translate into a generic evolution in the scaling-relation planes as well: a rapid transient roughly along the mass scaling relations, a subsequent slow drift across the scatter until virialization, followed by a slow evolution along and up the mass scaling relations as cooling recovers in the cluster cores. However, this drift is not sufficient to account for the observed scatter in the scaling relations. We also study the effects of mergers on several theoretical temperature measures of the intracluster medium: emission-weighted measures (T-ew), the spectroscopic-like measure (T-sl) proposed by Mazzotta et al. and plasma model fits to the integrated spectrum of the system (T-spec). We find that T-sl tracks T-spec for the entire duration of our mergers, illustrating that it remains a good tool for observational comparison even for highly disturbed systems. Furthermore, the transient temperature increases produced during first and second pericentric passage are 15-40 per cent larger for T-ew than for T-sl or T-spec. This suggests that the effects of transient temperature increases on sigma(8) and Omega(M) derived by Randall et al. are over estimated. Lastly, we examine the X-ray SZ proxy proposed by Kravtsov, Vikhlinin & Nagai (2006) and find that the tight mass scaling relation they predict remains secure through the entire duration of a merger event, independent of projection effects.
引用
收藏
页码:437 / 454
页数:18
相关论文
共 59 条
[1]   Physical implications of the X-ray properties of galaxy groups and clusters [J].
Babul, A ;
Balogh, ML ;
Lewis, GF ;
Poole, GB .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 330 (02) :329-343
[2]   An analytic investigation of the scatter in the integrated X-ray properties of galaxy groups and clusters [J].
Balogh, ML ;
Babul, A ;
Voit, GM ;
McCarthy, IG ;
Jones, LR ;
Lewis, GF ;
Ebeling, H .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 366 (02) :624-634
[3]  
BARTELMANN M, 1996, MNRAS, V23, P431
[4]   Measurements of Sunyaev-Zel'dovich effect scaling relations for clusters of galaxies [J].
Benson, BA ;
Church, SE ;
Ade, PAR ;
Bock, JJ ;
Ganga, KM ;
Henson, CN ;
Thompson, KL .
ASTROPHYSICAL JOURNAL, 2004, 617 (02) :829-846
[5]   X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation [J].
Borgani, S ;
Murante, G ;
Springel, V ;
Diaferio, A ;
Dolag, K ;
Moscardini, L ;
Tormen, G ;
Tornatore, L ;
Tozzi, P .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2004, 348 (03) :1078-1096
[6]  
BURNS JO, 2006, ASTROPH0610850
[7]   The SZ effect as a probe of non-gravitational entropy in groups and clusters of galaxies [J].
Cavaliere, A ;
Menci, N .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2001, 327 (02) :488-498
[8]   The formation histories of galaxy clusters [J].
Cohn, JD ;
White, M .
ASTROPARTICLE PHYSICS, 2005, 24 (4-5) :316-333
[9]   COOLING FLOWS AND THE X-RAY LUMINOSITY TEMPERATURE RELATION FOR CLUSTERS [J].
FABIAN, AC ;
CRAWFORD, CS ;
EDGE, AC ;
MUSHOTZKY, RF .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1994, 267 (03) :779-784
[10]   XMM-Newton study of the two-dimensional structure of the REFLEX-DXL galaxy clusters [J].
Finoguenov, A ;
Böhringer, H ;
Zhang, YY .
ASTRONOMY & ASTROPHYSICS, 2005, 442 (03) :827-+