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COLD FRONTS IN GROUPS AND CLUSTERS AND THEIR DYNAMICAL STATE IN THE OPTICAL

COLD FRONTS IN GROUPS AND CLUSTERS AND THEIR DYNAMICAL STATE IN THE OPTICAL. FABIO GASTALDELLO INAF-IASF MILAN & UC IRVINE M. MESSA, L. DI GESU S. GHIZZARDI, M. ROSSETTI, D. BUOTE, S. ETTORI, F. BRIGHENTI, W. MATHEWS. INTRO: SLOSHING COLD FRONTS AND OBSERVABLE EFFECTS

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COLD FRONTS IN GROUPS AND CLUSTERS AND THEIR DYNAMICAL STATE IN THE OPTICAL

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  1. COLD FRONTS IN GROUPS AND CLUSTERS AND THEIR DYNAMICAL STATE IN THE OPTICAL FABIO GASTALDELLO INAF-IASF MILAN & UC IRVINE M. MESSA, L. DI GESU S. GHIZZARDI, M. ROSSETTI, D. BUOTE, S. ETTORI, F. BRIGHENTI, W. MATHEWS

  2. INTRO: SLOSHING COLD FRONTS AND OBSERVABLE EFFECTS • SLOSHING COLD FRONTS IN THE RELAXED GROUPS NGC 5044 AND IC 1860 • PECULIAR VELOCITY OF BCGs AND X-RAY THERMODYNAMICAL STATE / PRESENCE OF CFs OUTLINE

  3. COLD FRONTS IN CLUSTERS IN MERGING CLUSTERS IN RELAXED CLUSTERS Markevitch & Vikhlinin 07

  4. SLOSHING CFs IN CLUSTERS Ascasibar & Markevitch 06

  5. SLOSHING CFs IN CLUSTERS • SB DISCONTUINITIES, SPIRAL FEATURES IN T • STEEP ENTROPY GRADIENT • cD PECULIAR VELOCITY • ABUNDANCE DISCONTUINITIES Ascasibar & Markevitch 06

  6. HOW ABOUT GROUPS ? EXAMPLES IN MERGING SYSTEMS, e.g. NGC 1404 IN FORNAX (Machacek+05)

  7. SLOSHING CFs IN NGC 5044 z=0.009 kT=1.2 keV Gastaldello+09

  8. MENDEL+08 STUDY OF 111 MEMBERS: PECULIAR VELOCITY OF 150 km/s WRT THE MEAN VELOCITY SLOSHING CFs IN NGC 5044

  9. SLOSHING CFs IN NGC 5044 DETECTION OF A SUBSTRUCTURE (99.9 %) AT 1.4 Mpc MENDEL+08. OR NGC 5054 (DAVID+09).

  10. z=0.022 kT=1.4 keV SLOSHING CFs IN IC 1860 Di Gesu, FG, et al. in prep

  11. SLOSHING CFs IN IC 1860 Di Gesu, FG, et al. in prep

  12. SLOSHING CFs IN IC 1860 PRELIMINARY MODELING CONSISTENT WITH DENSITY JUMP OF 1.4.

  13. SLOSHING CFs IN IC 1860 STUDY OF 81 MEMBERS AVAILABLE IN NED: PECULIAR VELOCITY OF 100 km/s WRT THE MEAN VELOCITY

  14. SLOSHING CFs IN IC 1860 SUBSTRUCTURE PRESENT AT THE 98.2 % LEVEL

  15. COZIOL+09 452 ABELL CLUSTERS W/ MORE THAN 10 MEMBERS VP OF BCG CAVAGNOLO+09 241 CLUSTERS K0 AS INDICATOR OF THERMODYNAMICAL STATE PECULIAR VELOCITIES OF BCGs AND X-RAY STATE CROSS-MATCH OF X-RAY PEAK AND BCG POSITION. ONLY IN EXTREME MERGERS (A754, A3376) LARGE SEPARATION. RESULTING SAMPLE OF 54 OBJECTS FG, Messa, et al. in prep

  16. NCC CC PECULIAR VELOCITIES OF BCGs AND X-RAY STATE

  17. With CF NO CF VPEC OF BCGs AND X-RAY STATE A133 176 A1644 29 A1795 238 A496 55 A2029 61 A2052 185 A2199 156 CENTAURUS 125 A4059 27 A85 43 A478 340 A1068 127 A2107 187 A2556 85 A2626 802 A2717 107 A3112 215 A3581 31 ESO 3060170 20 MKW3S 27 A1361 204 A2667 382

  18. ABELL 2626 82 MEMBERS CLEAR DETECTION OF SUBSTRUCTURES ALREADY IN MOHR+96 IT HOSTS A MINI RADIO HALO (GITTI+04) PEAK 1 CAVEAT: SUBSTRUCTURES ! PEAK 2 vcl: 17307 km/s  16533 km/s Vp: 802 km/s  27 km/s σv: 1057 km/s  658 km/s kT=2.9 keV

  19. COZIOL+09: “A large fractions of BCGs have significant peculiar velocity. This has one immediate consequence, which is that most clusters harboring a dominant galaxy are not dynamically relaxed” VAN DEN BOSCH+05: “The brightest galaxy in a dark matter halo is expected to reside at rest at the centre of the halo. In this paper, we test this `Central Galaxy Paradigm' (CGP) using group catalogues extracted from the Two-Degree Field Galaxy Redshift Survey (2dFGRS) and the Sloan Digital Sky Survey (SDSS). VPEC OF BCGs: SOME PEOPLE SAY ... We show that the CGP is only consistent with the data in haloes with M < 1013 Msun, while in more massive haloes the data indicate a non-zero offset between the brightest galaxy and the satellites. This indicates that either central galaxies reside at the minimum of the dark matter potential, but that the halo itself is not yet fully relaxed, or, that the halo is relaxed, but that the central galaxy oscillates in its potential well.

  20. MIRALDA-ESCUDE’+95: “The fact that cD galaxies often have large peculiar velocities relative to the average of the cluster galaxies has been used as an argument against their identification as cluster centers: however, clusters are continuously merging, and their density peaks do not need to coincide with their centers of mass. Substructure will cause the density peaks to move, in response to the gravitational forces of the infalling material” VPEC OF BCGs: SOME PEOPLE SAY ...

  21. SLOSHING COLD FRONTS ARE STARTING TO BE DETECTED IN AN INCREASING NUMBER OF GROUPS: FEATURE PRESENT AT ALL SCALES (see also NGC 5098: Randall+09, NGC 5846: Machaceck poster) • OFF-AXIS MERGERS INDUCING COLD FRONTS CAN EXPLAIN SPEEDING BCGs ALSO IN RELAXED CLUSTERS: NEEDS FURTHER INVESTIGATION TAKING CARE OF POSSIBLE SUBSTRUCTURES SUMMARY

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