Proposal ID | 030569 |
Title | Mapping observation of dynamical structures in the Perseus cluster |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305690101 |
DOI | https://doi.org/10.5270/esa-jj8ngmq |
Principal Investigator, PI | Dr Tae Furusho |
Abstract | XMM-Newton performed 5 pointing observations in the Perseus cluster, and showedvery interesting features in the large-scale distributions of temperature. It iscertain that the cluster is undergoing at least 2 major mergers. We propose here5 further pointings to fill up the bright part of the cluster emission, whichwill give us full views on the 2 mergers going on in the southwest (IC 310subcluster) and in the east (extended cool subcluster) of the Perseus system.The data will show us a complete view about the substructures, with the gasheating and mixing processes taking place in this massive system. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2006-02-10T17:26:25Z/2006-02-11T18:32:16Z |
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 | 2007-03-03T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "cool subcluster", "scale distributions", "perseus system", "gas heating", "perseus cluster", "XMM-Newton", "xmm newton performed", "mixing processes taking", "cluster emission", "XMM", "major mergers", "massive system", "dynamical structures" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Tae Furusho, 2007, 'Mapping observation of dynamical structures in the Perseus cluster', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jj8ngmq |