Cold fronts and multi-temperature structures in the core of Abell 2052
arXiv:1008.3109 · doi:10.1051/0004-6361/201015198
Abstract
The physics of the coolest phases in the hot Intra-Cluster Medium (ICM) of clusters of galaxies is yet to be fully unveiled. X-ray cavities blown by the central Active Galactic Nucleus (AGN) contain enough energy to heat the surrounding gas and stop cooling, but locally blobs or filaments of gas appear to be able to cool to low temperatures of 10^4 K. In X-rays, however, gas with temperatures lower than 0.5 keV is not observed. Using a deep XMM-Newton observation of the cluster of galaxies Abell 2052, we derive 2D maps of the temperature, entropy, and iron abundance in the core region. About 130 kpc South-West of the central galaxy, we discover a discontinuity in the surface brightness of the hot gas which is consistent with a cold front. Interestingly, the iron abundance jumps from ~0.75 to ~0.5 across the front. In a smaller region to the North-West of the central galaxy we find a relatively high contribution of cool 0.5 keV gas, but no X-ray emitting gas is detected below that temperature. However, the region appears to be associated with much cooler H-alpha filaments in the optical waveband. The elliptical shape of the cold front in the SW of the cluster suggests that the front is caused by sloshing of the hot gas in the clusters gravitational potential. This effect is probably an important mechanism to transport metals from the core region to the outer parts of the cluster. The smooth temperature profile across the sharp jump in the metalicity indicates the presence of heat conduction and the lack of mixing across the discontinuity. The cool blob of gas NW of the central galaxy was probably pushed away from the core and squeezed by the adjacent bubble, where it can cool efficiently and relatively undisturbed by the AGN. Shock induced mixing between the two phases may cause the 0.5 keV gas to cool non-radiatively and explain our non-detection of gas below 0.5 keV.
11 pages, 9 figures, A&A, in press
References in corpus (45)
- Star Formation in Galaxies Along the Hubble Sequence
- The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections
- Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations
- A Systematic Study of Radio-Induced X-ray Cavities in Clusters, Groups, and Galaxies
- Shocks and cold fronts in galaxy clusters
- Chandra X-ray Observations of the Hydra A Cluster: An Interaction Between the Radio Source and the X-Ray-Emitting Gas
- High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies
- X-ray Imaging Spectroscopy of Abell 1835
- The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton
- A Catalog of Galaxy Clusters Observed by XMM-Newton
- X-ray Spectroscopy of the Cluster of Galaxies Abell 1795 with XMM-Newton
- Cooling Flows as a Calorimeter of AGN Mechanical Power
- The origin of cold fronts in the cores of relaxed galaxy clusters
- Chandra Observation of the Radio Source / X-ray Gas Interaction in the Cooling Flow Cluster Abell 2052
- The relationship between the optical Halpha filaments and the X-ray emission in the core of the Perseus cluster
- A deeper X-ray study of the core of the Perseus galaxy cluster: the power of sound waves and the distribution of metals and cosmic rays
- Hot Bubbles from Active Galactic Nuclei as a Heat Source in Cooling Flow Clusters
- Spatially resolved X-ray spectroscopy of cooling clusters of galaxies
- Adaptive Binning of X-ray data with Weighted Voronoi Tesselations
- Non-hydrostatic gas in the core of the relaxed galaxy cluster A1795
- XMM-Newton observations of the cluster of galaxies Sersic 159-03
- On the Origin of the Extended Halpha Filaments in Cooling Flow Clusters
- Magnetic support of the optical emission line filaments in NGC 1275
- Chandra Observation of the Cooling Flow Cluster Abell 2052
- Collisional heating as the origin of filament emission in galaxy clusters
- Mapping small-scale temperature and abundance structures in the core of the Perseus cluster
- Chandra constraints on the thermal conduction in the intracluster plasma of A2142
- Spatially-resolved X-ray spectroscopy of the core of the Centaurus cluster
- Chandra Imaging of the X-ray Core of the Virgo Cluster
- Constraining supernova models using the hot gas in clusters of galaxies
- Thermal Instability with Anisotropic Thermal Conduction and Adiabatic Cosmic Rays: Implications for Cold Filaments in Galaxy Clusters
- The elemental abundances in the intracluster medium as observed with XMM-Newton
- Temperature and Heavy Element Abundance Profiles of Cool Clusters of Galaxies from ASCA
- Metal-rich multi-phase gas in M87: AGN-driven metal transport, magnetic-field supported multi-temperature gas, and constraints on non-thermal emission observed with XMM-Newton
- Feedback under the microscope II: heating, gas uplift, and mixing in the nearest cluster core
- Cluster mergers, core oscillations, and cold fronts
- XMM-Newton Spectroscopy of the Cluster of Galaxies 2A 0335+096
- Chemical evolution in Sersic 159-03 observed with XMM-Newton
- Deep high-resolution X-ray spectra from cool-core clusters
- The extended H-alpha emitting filaments surrounding NGC4696, the central galaxy of the Centaurus cluster
- X-ray and Optical Filaments in M87
- X-ray spectroscopy on Abell 478 with XMM-Newton
- Shocks and Bubbles in a Deep Chandra Observation of the Cooling Flow Cluster Abell 2052
- Feedback through multiple outbursts in the cluster 2A 0335+096
- The temperature structure in the core of Sersic 159-03
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- How Much Can We Learn From A Merging Cold Front Cluster? : Insights From X-ray Temperature and Radio Maps of Abell 3667
- Merging cold front and AGN feedback in the peculiar galaxy cluster Abell 2626
- AGN feedback and iron enrichment in the powerful radio galaxy, 4C+55.16
- The metal contents of two groups of galaxies
- Heating and enriching the intracluster medium
- Strong Magnetization Measured in the Cool Cores of Galaxy Clusters
- Metal jumps across sloshing cold fronts: the case of A496
- Deprojecting galaxy-cluster cold fronts: evidence for bulk, magnetised spiral flows
- Chandra observation of a cold front in Abell 2554
- Advection by large-scale spiral flows in galaxy clusters
- The strongest cool core in REXCESS: Missing X-ray cavities in RXC J2014.8-2430
- The clus model in SPEX: projection and resonant scattering effects on the iron abundance and temperature profiles of galaxy clusters
- Imaging-spectroscopy diagnosis of the giant sloshing spiral in the Virgo cluster with the Einstein Probe Follow-up X-ray Telescope
- On the Origin of Diffuse Radio Emission in Abell 85 -- Insights from new GMRT Observations
- Evidence of sloshing-driven mini-halo formation in the cool-core cluster RXCJ1558.3-1410