2010ApJ...716..739M


Query : 2010ApJ...716..739M

2010ApJ...716..739M - Astrophys. J., 716, 739-745 (2010/June-2)

Implications of a high angular resolution image of the Sunyaev-Zel'Dovich effect in RXJ1347-1145.

MASON B.S., DICKER S.R., KORNGUT P.M., DEVLIN M.J., COTTON W.D., KOCH P.M., MOLNAR S.M., SIEVERS J., AGUIRRE J.E., BENFORD D., STAGUHN J.G., MOSELEY H., IRWIN K.D. and ADE P.

Abstract (from CDS):

The most X-ray luminous cluster known, RXJ1347-1145 (z = 0.45), has been the object of extensive study across the electromagnetic spectrum. We have imaged the Sunyaev-Zel'dovich effect (SZE) at 90 GHz (λ = 3.3 mm) in RXJ1347-1145 at 10'' resolution with the 64 pixel MUSTANG bolometer array on the Green Bank Telescope, confirming a previously reported strong, localized enhancement of the SZE 20'' to the southeast of the center of X-ray emission. This enhancement of the SZE has been interpreted as shock-heated (>20 keV) gas caused by an ongoing major (low mass ratio) merger event. Our data support this interpretation. We also detect a pronounced asymmetry in the projected cluster pressure profile, with the pressure just east of the cluster core ∼1.6x higher than just to the west. This is the highest resolution image of the SZE made to date.

Abstract Copyright: ∼

Journal keyword(s): cosmic background radiation - cosmology: observations - galaxies: clusters: individual: RXJ1347-1145

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 ClG 0657-56 ClG 06 58 26.9 -55 58 21           ~ 1077 1
2 3C 279 Bla 12 56 11.16657958 -05 47 21.5251510   18.01 17.75 15.87   ~ 3205 2
3 ClG J1347-1145 ClG 13 47 30.5 -11 45 07           ~ 577 0
4 V* V1610 Cyg pA* 21 02 18.27 +36 41 37.0           F5Iae 892 1

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