A dataset provided by the European Space Agency

Name 074512
Title Understanding the merger geometry and the complex relic system in Abell 3411


DOI 10.5270/esa-oontvv2
Author Ms Georgiana Ancuta Ogrean
Description Galaxy cluster mergers trigger Mpc-scaled shocks in the ICM, which can accelerate particles to relativistic energies to form arc-shaped radio relics. Last year, we discovered a spectacular radio relic in the Planck cluster A3411. The relic has a fragmentary morphology, at odds with the arc-shaped shocks predicted by hydrodynamical simulations. We propose for a 200 ks XMM observation to detect and characterize the shock at the radio relic. The combination of X-ray and radio data will provide the opportunity to (1) determine the shape of the shock surface; (2) model the merger event; and (3) test different shock acceleration models. Data on such puzzling objects is crucial to our understanding of relics.
Publication The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
X-Ray Morphological Analysis of the Planck ESZ Clusters . Lovisari, Lorenzo, Forman, William R., et all. . ApJ . 846-51 . 2017 . 2017ApJ...846...51L ,
X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton . Lovisari, Lorenzo, Schellenberger, Gerrit, et all. . ApJ . 892-102 . 2020 . 2020ApJ...892..102L ,
X-ray study of the merging galaxy cluster Abell 3411-3412 with XMM-Newton and Suzaku . Zhang, X., Simionescu, A., et all. . A&A . 642-89 . 2020 . 2020A&A...642A..89Z ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-11-18T14:07:48Z/2014-11-20T04:11:08Z
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 2015-12-05T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-12-05T23:00:00Z, 074512, 17.56_20190403_1200. https://doi.org/10.5270/esa-oontvv2