A dataset provided by the European Space Agency

Name: The Role of AGN Feedback in Massive Elliptical Galaxies
Published: 2012-07-28T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	067287
Title	The Role of AGN Feedback in Massive Elliptical Galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672870101
DOI	https://doi.org/10.5270/esa-ac04b57
Principal Investigator, PI	Dr Zhiyuan Li
Abstract	We propose a 70 ks XMM-Newton observation of the hot gas around the unusualradio galaxy IC 4296 (PKS 1333-33) to measure the thermodynamic parameters ofthe hot gas environment. This massive elliptical galaxy lies at the center of anearby group, and has a variety of unusual features suggesting a stronginteraction between the jet and the ambient gas. On 100-kpc scales, the jetsterminate in a mildly edge-brightened radio lobes without a conspicuous hotspot, suggestive of efficient subsonic thermalization of the jet flow. Strongexternal shocks have been found in systems with similar morphologies (e.g.Centaurus A). Understanding the role of AGN feedback has important implicationsto our fundamental knowledge of galaxy evolution.
Publications	A volume-limited sample of X-ray galaxy groups and clusters - I. Radial entropy and cooling time profiles \|Panagoulia E. K. Fabian A. C. \| MNRAS \| 438-2341 \| 2014 \| 2014MNRAS.438.2341P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.2341P 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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y A volume-limited sample of X-ray galaxy groups and clusters - II. X-ray cavity dynamics \|Panagoulia E. K. Fabian A. C. et al. \| MNRAS \| 444-1236 \| 2014 \| 2014MNRAS.444.1236P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444.1236P The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Correlation between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies \|Bogdan Akos Lovisari Lorenzo et al. \| ApJ \| 852-131 \| 2018 \| 2018ApJ...852..131B \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...852..131B The non-uniformity of galaxy cluster metallicity profiles \|Lovisari L. Reiprich T. H. \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L A new clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw H. P. Roberts T. P. et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E Powerful AGN jets and unbalanced cooling in the hot atmosphere of IC 4296 \|Grossova R. Werner N. et al. \| MNRAS \| 488-1917 \| 2019 \| 2019MNRAS.488.1917G \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.488.1917G Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations \|Bassini L. Rasia E. et al. \| A&A \| 630-144 \| 2019 \| 2019A&A...630A.144B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...630A.144B A new multiwavelength census of blazars \|Paggi A. Bonato M. et al. \| A&A \| 641-62 \| 2020 \| 2020A&A...641A..62P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...641A..62P Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z An XMM-Newton Early-type Galaxy Atlas \|Islam Nazma Kim Dong-Woo et al. \| ApJS \| 256-22 \| 2021 \| 2021ApJS..256...22I \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..256...22I The impact of precession on the observed population of ULXs \|Khan Norman Middleton Matthew J. et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K Very Large Array Radio Study of a Sample of Nearby X-Ray and Optically Bright Early-type Galaxies \|Grossovu00e1 Romana Werner Norbert et al. \| ApJS \| 258-30 \| 2022 \| 2022ApJS..258...30G \| http://ui.adsabs.harvard.edu/#abs/2022ApJS..258...30G The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows R. Comerford Julia M. et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D Black Hole Mass Determination Using X-ray Data \|Jang Insuk \| PhDT \| 0-58 \| 2014 \| 2014PhDT........58J \| http://ui.adsabs.harvard.edu/#abs/2014PhDT........58J New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2011-07-11T11:56:04Z/2011-07-12T07:54:42Z
Version	21.51_20241115_1113
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	2012-07-28T00:00:00Z
Last Update	2026-07-09
Keywords	"ambient gas", "fundamental knowledge", "thermodynamic parameters", "jets terminate", "XMM-Newton", "galaxy evolution", "hot gas", "agn feedback", "XMM", "external shoc", "massive elliptical galaxy", "jet flow", "efficient subsonic thermalization", "radiogalaxy ic 4296", "xmm newton", "conspicuous hot spot"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Zhiyuan Li, 2012, 'The Role of AGN Feedback in Massive Elliptical Galaxies', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-ac04b57
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.