A dataset provided by the European Space Agency

Name 065403
Title Diffusive shock acceleration induced by a cluster merger?


DOI 10.5270/esa-5h8nwed
Author Prof Huub Rottgering
Description We have discovered an extraordinarily long, narrow steep spectrum radio relic in the galaxy cluster CIZA J2242.8+5301. The relic has a remarkable radio spectral index gradient perpendicular to its long axis and polarization points to a magnetic field parallel to it. Here we propose deep X-ray observations to (i) confirm the presence of a shock front at the position of the radio relic, (ii) determine the shock physical conditions, (iii) characterize the dynamical state of the cluster, and (iv) map the temperature distribution. These observations will (i) provide conclusive evidence for the existence of diffusive shock acceleration and, (ii) constrain scenarios connecting the properties of shock fronts, particle acceleration mechanisms, and the occurrence of radio relics.
Publication XMM-Newton observations of the merging galaxy cluster CIZA J2242.8+5301 . Ogrean, G. A., Bruggen, M., et all. . MNRAS . 429-2617 . 2013 . 2013MNRAS.429.2617O ,
X-ray observations of the merging cluster CIZA J2242.8+5301 . Ogrean, G., Bruggen, M., et all. . AN . 334-342 . 2013 . 2013AN....334..342O ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Suzaku X-ray study of the double radio relic galaxy cluster CIZA J2242.8+5301 . Akamatsu, H., van Weeren, R. J., et all. . A&A . 582-87 . 2015 . 2015A&A...582A..87A ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Iron abundance distribution in the hot gas of merging galaxy clusters . Urdampilleta, I., Mernier, F., et all. . A&A . 629-31 . 2019 . 2019A&A...629A..31U ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-12-13T16:30:27Z/2010-12-15T06:19:14Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2012-01-22T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-01-22T00:00:00Z, 065403, 17.56_20190403_1200. https://doi.org/10.5270/esa-5h8nwed