| Proposal ID | 030035 |
| Title | The Physics of Cooling Flow Clusters with Central Radio Sources |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300350301 |
| DOI | https://doi.org/10.5270/esa-3e142wn |
| Principal Investigator, PI | Dr Craig Sarazin |
| Abstract | Central galaxies in rich clusters are the sites of cluster cooling flows, withlarge masses of gas cooling through part of the X-ray band. Many of thesegalaxies host powerful radio sources. These sources can displace and compressthe X-ray gas leading to enhanced cooling and star formation. We proposeobservations of two bright cooling flows (A1367 & A2147) with radio sources thatwill exploit the large collecting area and spectral resolution of XMM-Newton. Wewill constrain the source of additional pressure in radio holes in the X-rayemission needed to support overlying shells of X-ray gas. We will address theproblem of the lack of kT less than 1-2 keV gas in cooling flows by searchingfor abundance inhomogeneities, heating from the radio source, and excess absorption. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2006-02-02T01:25:47Z/2006-02-04T04:39:42Z |
| 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 | 2007-02-19T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "excess absorption", "kev gas", "xmm newton", "additional pressure", "xray gas", "spectral resolution", "cluster cooling flows", "radio source", "xray emission", "radio sources", "xray band", "cooling flows", "enhanced cooling", "gas cooling", "powerful radio sources", "XMM-Newton", "central galaxy", "abundance inhomogeneities", "rich cluster", "xray gas leading", "star formation", "central radio sources", "support overlying shells", "cooling flow cluster", "XMM" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Craig Sarazin, 2007, 'The Physics of Cooling Flow Clusters with Central Radio Sources', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3e142wn |