A dataset provided by the European Space Agency

Name 065272
Title Cavities, strong shocks and AGN heating in galaxy groups
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652720101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652720201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652720301

DOI 10.5270/esa-7243lth
Author Dr Ming Sun
Description Outbursts of SMBHs have significant impact on structure formation and evolution. Their imprint on ICM (cavities, shocks and ^ated entropy) provides an historical chronicle of the SMBH activity. However, AGN heating has not been well studied in groups (especially for groups hosting strong radio AGN), although it should affect the group gas much more than the cluster gas. We propose XMM observations of two groups with strong radio AGN. Both have clear features indicative of heating from the radio AGN in short XMM or Chandra exposures. The results will fill the little explored regime of the L_radio - L_power plane for groups. One galaxy also has a mysterious emission line in the spectrum of its AGN, which needs to be tested and studied with deeper data.
Publication A multi-wavelength study of nuclear activity and environment of low-power radio galaxy CTD 86 . Pandge, M. B., Dewangan, G. C., et all. . MNRAS . 435-3385 . 2013 . 2013MNRAS.435.3385P ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton . Svoboda, J., Guainazzi, M., . A&A . 603-127 . 2017 . 2017A&A...603A.127S ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-06-21T04:54:40Z/2011-03-09T00:08:32Z
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 2012-03-22T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-03-22T00:00:00Z, 065272, 17.56_20190403_1200. https://doi.org/10.5270/esa-7243lth