A dataset provided by the European Space Agency

Name 011226
Title Hierarchical Merging and the Intracluster Medium
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112260101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112260201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112260301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112260401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112260501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112260601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112260801

DOI https://doi.org/10.5270/esa-cwwyaay
Author European Space Agency
Description GT- Hierarchical merging implies that clusters are assembled by the merger
of smaller systems - however the effect of the merger process on clusters
and their galaxies is still poorly understood. We propose to use the EPIC
spectral imagers to map the state of the intracluster medium in a sample
consisting of the brightest merging clusters in the redshift range which is
optimum for XMM. These systems cover a range of merger stages, and of mass
ratios between the merging components. This will enable us to explore the
development of shock heating, cooling flow disruption, gas mixing and galaxy
stripping through the merger process. Such a study is essential if we are to
be able to model the evolution of clusters, and of the galaxies within them.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-08-17T22:50:07Z/2002-12-07T11:47:52Z
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 2004-01-30T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004, Hierarchical Merging And The Intracluster Medium, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-cwwyaay