A dataset provided by the European Space Agency

Name 020328
Title A SEARCH FOR THE GROUP ENVIRONMENTS OF LOW-POWER FRII RADIO GALAXIES
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203280101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203280201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203280301

DOI 10.5270/esa-pzf7yyj
Author Dr MARTIN HARDCASTLE
Description Although a good deal of indirect evidence points towards moderate or poor groups as the environment of low-luminosity (and therefore typical) FRII radio galaxies, there are almost no direct X-ray observations of the required hot, confining medium. An FRII radio source would have a dramatic effect on the gas in a group, heating and potentially expelling a significant fraction of it, with important consequences for our understanding of group evolution. In order to characterize the X-ray environments of typical FRII sources, we propose a small survey of the nearest few FRII sources of intermediate size drawn from the well-studied 3CRR catalogue. Our observations will allow us to detect, and measure the properties of, group-scale emission around our targets.
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-01-04T04:49:31Z/2004-05-02T10:54:30Z
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 2005-06-13T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-06-13T00:00:00Z, 020328, 17.56_20190403_1200. https://doi.org/10.5270/esa-pzf7yyj