A dataset provided by the European Space Agency

Name 014286
Title Hydrodynamics of Merging Clusters
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0142860201

DOI 10.5270/esa-vlqircj
Author Dr Laurence David
Description We propose to observe two clusters of galaxies that are undergoing major mergers (A2744 and A1758). These clusters were recently observed by Chandra and exhibit many of the classic features of merging systems: complex X-ray morphologies, NAT radio sources, and radio halos. While great advances have been made in observational cosmology over the past decade, there is still much to be learned about the hydrodynamic and relaxation processes that occur during and after cluster merging.Using the light gathering power of XMM-Newton, we can derive a high resolution temperature map and determine if the sharp features seen in the Chandra images are contact discontinuties or shocks, the shock strengths, and the time since the on-set of the merger.
Publication The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
The X-ray Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars . Young, M., Elvis, M., . ApJ . 708-1388 . 2010 . 2010ApJ...708.1388Y ,
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
New constraints on the X-ray spectral properties of type 1 active galactic nuclei . Scott, A. E., Stewart, G. C., et all. . MNRAS . 417-992 . 2011 . 2011MNRAS.417..992S ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
LoCuSS: A Comparison of Cluster Mass Measurements from XMM-Newton and Subaru---Testing Deviation from Hydrostatic Equilibrium and Non-thermal Pressure Support . Zhang, Yu-Ying, Okabe, Nobuhiro, et all. . ApJ . 711-1033 . 2010 . 2010ApJ...711.1033Z ,
LoCuSS: Calibrating Mass-observable Scaling Relations for Cluster Cosmology with Subaru Weak-lensing Observat...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-11-12T13:40:01Z/2002-11-13T05:33:38Z
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 2004-01-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-01-25T00:00:00Z, 014286, 17.56_20190403_1200. https://doi.org/10.5270/esa-vlqircj