Proposal ID | 040001 |
Title | The Abell 3395-Abell 3391 Filament in the Horologium Supercluster |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400010201 |
DOI | https://doi.org/10.5270/esa-lgewewj |
Principal Investigator, PI | Dr Mark Henriksen |
Abstract | We will use the spectro-spatial capability of XMM to map the hot gas of theentire Abell 3395-Abell 3391 region of the Horologium supercluster. Inparticular, we will: (1) measure the baryon fraction for clusters, groups, andfilamentary gas, (2) make temperature, pressure, and entropy maps to search forthe merger and infall signatures of the complex Abell 3395 3-body system, (3)construct a dynamical model of the Abell 3395-Abell 3391 filament using theX-ray measured masses combined with the galaxy kinematical parameters obtainedfrom Horologium Consortium collaborators, and (4) work with HorologiumConsortium members on a multi-waveband analysis of galaxy evolution in thecontext of large-scale structure formation. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2007-01-24T12:30:29Z/2007-04-06T11:59:47Z |
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 | 2008-04-20T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "horologium supercluster", "complex abell 3395", "infall signatures", "body system", "horologium consortium collaborators", "dynamical model", "spectro spatial", "galaxy evolution", "horologium consortium", "scale structure formation", "Abell 3395", "galaxy kinematical parameters", "baryon fraction", "masses combined", "entropy maps", "multi waveband analysis", "XMM", "filamentary gas", "hot gas" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Mark Henriksen, 2008, 'The Abell 3395-Abell 3391 Filament in the Horologium Supercluster', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-lgewewj |