A dataset provided by the European Space Agency

Name 030395
Title Giant Cavities and Large Scale Shocks in the Distant Cluster MS0735.6+7421
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303950101

DOI 10.5270/esa-rucypd4
Author Prof Brian McNamara
Description We propose to obtain a deep image of the redshift z=0.22 cluster MS0735.6+7421. The cluster.s enormous system of cavities and shocks are depositing 5-8E61erg into the ICM. Heating the cluster at a level of ~1-2 keV per particle, this is enough energy to quench a 200 M0-yr cooling flow for several Gyr and to .preheat. the cluster. The image will be used to examine the impact of AGN heating on the L-T relation, to constrain the temperature of the gas filling the cavities, to measure the temperature jump across the shock, and to search for evidence of earlier outbursts.
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 ,
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 ,
Cosmological Effects of Powerful AGN Outbursts in Galaxy Clusters: Insights from an XMM-Newton Observation of MS 0735+7421 . Gitti, M., McNamara, B. R., et all. . ApJ . 660-1118 . 2007 . 2007ApJ...660.1118G ,
X-Ray Absorption from the Milky Way Halo and the Local Group . Bregman, Joel N., Lloyd-Davies, Edward J., . ApJ . 669-990 . 2007 . 2007ApJ...669..990B ,
An Energetic AGN Outburst Powered by a Rapidly Spinning Supermassive Black Hole or an Accreting Ultramassive Black Hole . McNamara, B. R., Kazemzadeh, F., et all. . ApJ . 698-594 . 2009 . 2009ApJ...698..594M ,
Constraints on turbulent velocity broadening for a sample of clusters, groups and elliptical galaxies using XMM-Newton . Sanders, J. S., Fabian, A. C., . MNRAS . 410-1797 . 2011 . 2011MNRAS.410.1797S ,
Revealing O VII from stacked X-ray grating spectra of clusters, groups and elliptical ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-04-01T23:05:25Z/2005-04-02T19:02:24Z
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 2006-06-24T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-06-24T00:00:00Z, 030395, 17.56_20190403_1200. https://doi.org/10.5270/esa-rucypd4