Proposal ID | 010886 |
Title | Poor Groups Of Galaxies With Extended X-ray Emission |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108860101 |
DOI | https://doi.org/10.5270/esa-qsuwsp9 |
Principal Investigator, PI | Dr Richard Mushotzky |
Abstract | GT- Most galaxies belong to poor groups, and much of the baryonic matter incollapsed objects in the universe resides in the X-ray emitting intragroup medium. The distribution, and thermal and chemical properties of this hot gasprovides an ideal laboratory for testing theories of cD galaxy formation and theeffects of star-formation-driven feedback on intergalactic matter. We propose toobserved three very poor groups with extended X-ray emission peaked on a centralbright elliptical galaxy in order to measure the profiles of temperature andabundances of various elements, and decompose these into components associatedwith the central galaxy and the group as a whole. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2000-12-24T14:54:03Z/2002-07-08T00:10:19Z |
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 | 2003-09-04T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "xray emission peaked", "galaxy belong", "testing theories", "central galaxy", "chemical properties", "baryonic matter", "ideal laboratory", "universe resides", "xray emission", "cd galaxy formation", "intergalactic matter", "collapsed objects", "hot gas" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Richard Mushotzky, 2003, 'Poor Groups Of Galaxies With Extended X-ray Emission', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qsuwsp9 |