Proposal ID | 030395 |
Title | Giant Cavities and Large Scale Shocks in the Distant Cluster MS0735.6+7421 |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303950101 |
DOI | https://doi.org/10.5270/esa-rucypd4 |
Principal Investigator, PI | Prof Brian McNamara |
Abstract | We propose to obtain a deep image of the redshift z=0.22 cluster MS0735.6+7421.The clusters enormous system of cavities and shocks are depositing 5-8E61erginto the ICM. Heating the cluster at a level of ~1/2 keV per particle, this isenough energy to quench a 200 M0/yr cooling flow for several Gyr and topreheat the cluster. The image will be used to examine the impact of AGNheating on the L-T relation, to constrain the temperature of the gas filling thecavities, to measure the temperature jump across the shock, and to search forevidence of earlier outbursts. |
Publications |
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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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 |
Last Update | 2025-01-27 |
Keywords | "distant cluster ms0735", "redshift z", "yr cooling flow", "temperature jump", "agn heating", "giant cavities", "cluster ms0735", "M0", "scale shoc", "gas filling", "deep image" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Prof Brian McNamara, 2006, 'Giant Cavities and Large Scale Shocks in the Distant Cluster MS0735.6+7421', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rucypd4 |