A dataset provided by the European Space Agency

Name 067467
Title Abell 545 an uncommon merging cluster
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674670101

DOI 10.5270/esa-248m35d
Author Dr Sabrina De Grandi
Description Detailed studies of A545 at radio, optical and X-ray wavelengths point to a system undergoing a major merger. The unique discovery of an extended stellar halo resembling that of a cD but with no associated BCG is particularly intriguing as it suggests this system may be undergoing a critical dynamic phase that is rarely observed. The available XMM data while hinting to a number of interesting features, most notably a shock ~400 kpc North of the surface brightness peak, are of limited use because of the extreme contamination by soft protons. We propose a 50 ks observation of A545 to constrain the phase and geometry of the merger. The combination of the proposed X-ray observation with the available optical and radio data will allow us to construct a global picture of the dynamical status of A545.
Publication 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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton . Svoboda, J., Guainazzi, M., . A&A . 603-127 . 2017 . 2017A&A...603A.127S ,
On the Connection between Turbulent Motions and Particle Acceleration in Galaxy Clusters . Eckert, D., Gaspari, M., et all. . ApJ . 843-29 . 2017 . 2017ApJ...843L..29E ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-08-30T10:25:18Z/2011-08-31T00:50:36Z
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 2012-09-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-09-29T00:00:00Z, 067467, 17.56_20190403_1200. https://doi.org/10.5270/esa-248m35d