Proposal ID | 014138 |
Title | SPATIAL ORIGIN OF THE NON-THERMAL X-RAY EMISSION IN THE CLUSTER A2256 |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0141380101 |
DOI | https://doi.org/10.5270/esa-39uk5wz |
Principal Investigator, PI | Dr Roberto Fusco-Femiano |
Abstract | We propose to observe the northwest radio relic of the cluster Abell 2256 for40 ksec in order to localize the non-thermal hard X-ray emission recentlydetected by BeppoSAX. The energy range and the spectral capabilities of EPICare able to detect the non-thermal radiation considering the low gas temperatureof the relic likely associated with the ongoing merger of a subcluster with themain cluster. Besides, we can firmly verify the suggested link between particleacceleration processes due to merger events and the formation of extended radioregions and non-thermal X-ray emission. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2003-04-27T13:44:43Z/2003-06-30T16:45:48Z |
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 | 2004-09-03T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "main cluster", "EPIC", "nonthermal xray emission", "Abell 2256", "energy range", "merger events", "low gas temperature", "suggested link", "spatial origin", "BeppoSAX", "nonthermal radiation", "cluster abell 2256", "northwest radio relic", "cluster a2256", "particle acceleration processes", "radio region" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Roberto Fusco-Femiano, 2004, 'SPATIAL ORIGIN OF THE NON-THERMAL X-RAY EMISSION IN THE CLUSTER A2256', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-39uk5wz |