A dataset provided by the European Space Agency

Name 000296
Title What disrupts the jets in wide-angle tail radio galaxies - testing merger models
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0002960101

DOI 10.5270/esa-jyhoyri
Author Dr Martin Hardcastle
Description Wide-angle tail radio galaxies (WATs) are a challenge to our understanding of the way in which extragalactic radio sources interact with their environment. Neither the disruption of their jets nor the 100-kpc-scale bending of their tails is fully understood. WATs always inhabit X-ray-luminous clusters, and recent cluster merger events may give rise to observed clumpy X-ray emission and to large-scale winds that bend and disrupt the jets. We propose to test this model in a small sample of well-studied WATs. XMM.s high sensitivity and spatial resolution will allow us to determine the nature of the clumpy gas and
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The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
Evidence for Rapidly Rotating Black Holes in Fanaroff-Riley I Radio Galaxies . Wu, Qingwen, Cao, Xinwu, . ApJ . 735-50 . 2011 . 2011ApJ...735...50W ,
Obscuration and Origin of Nuclear X-Ray Emission in FR I Radio Galaxies . Donato, D., Sambruna, R. M., . ApJ . 617-915 . 2004 . ...,
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Chandra and XMM-Newton Observations of a Sample of Low-Redshift FR I and FR II Radio Galaxy Nuclei . Evans, D. A., Worrall, D. M., et all. . ApJ . 642-96 . 2006 . 2006ApJ...642...96E ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Fe Kalpha line profile in AGNs: average shape and redshift dependence . Mao, Wei-Ming, Hu, Chen, et all. . RAA . 10-905 . 2010 . 2010RAA....10..905M ,
A Limit on the Number of Isolated Neutron Stars Detected in the ROSAT All-Sky-Survey Bright Source Catalog . Turner, Monica L., Rutledge, Robert E., et all. . ApJ . 714-1424 . 2010 . 2010ApJ...714.1424T ,
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Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 2012MNRAS.426..903P ,
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The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
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Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-06-22T05:08:28Z/2002-06-22T08:20:53Z
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 2003-08-06T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-08-06T00:00:00Z, 000296, 17.56_20190403_1200. https://doi.org/10.5270/esa-jyhoyri