| タイトル | Implications of a High Angular Resolution Image of the Sunyaev-Zel'Dovich Effect in RXJ1347-1145 |
| 著者（英） | Irwin, K. D.; Mason, B. S.; Ade, P.; Devlin, M.; Molnar, S. M.; Korngut, P. M.; Aguirre, J. E.; Cotton, W. D.; Moseley, H.; Dicker, S. R.; Sievers, J.; Koch, P. M.; Staguhn, J. G.; Benford, D. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2010-06-01 |
| 言語 | eng |
| 内容記述 | 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 (lambda = 33 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 (>20keV) 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 approx. 1.6x higher than just to the west. This is the highest resolution image of the SZE made to date. |
| NASA分類 | Astrophysics |
| 権利 | Copyright |
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