A dataset provided by the European Space Agency

Name 067287
Title The Role of AGN Feedback in Massive Elliptical Galaxies


DOI 10.5270/esa-ac04b57
Author Dr Zhiyuan Li
Description We propose a 70 ks XMM-Newton observation of the hot gas around the unusual radio galaxy IC 4296 (PKS 1333-33) to measure the thermodynamic parameters of the hot gas environment. This massive elliptical galaxy lies at the center of a nearby group, and has a variety of unusual features suggesting a strong interaction between the jet and the ambient gas. On 100-kpc scales, the jets terminate in a mildly edge-brightened radio lobes without a conspicuous hot spot, suggestive of efficient subsonic thermalization of the jet flow. Strong external shocks have been found in systems with similar morphologies (e.g. Centaurus A). Understanding the role of AGN feedback has important implications to our fundamental knowledge of galaxy evolution.
Publication 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 ,
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 ,
A volume-limited sample of X-ray galaxy groups and clusters - II. X-ray cavity dynamics . Panagoulia, E. K., Fabian, A. C., et all. . MNRAS . 444-1236 . 2014 . 2014MNRAS.444.1236P ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 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 all. . ApJ . 852-131 . 2018 . 2018ApJ...852..131B ,
The non-uniformity of galaxy cluster metallicity profiles . Lovisari, L., Reiprich, T. H., . MNRAS . 483-540 . 2019 . 2019MNRAS.483..540L ,
A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies . Earnshaw, H. P., Roberts, T. P., et all. . MNRAS . 483-5554 . 2019 . 2019MNRAS.483.5554E ,
Powerful AGN jets and unbalanced cooling in the hot atmosphere of IC 4296 . Grossova, R., Werner, N., et all. . MNRAS . 488-1917 . 2019 . ...,
Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations . Bassini, L., Rasia, E., et all. . A&A . 630-144 . 2019 . 2019A&A...630A.144B ,
A new multiwavelength census of blazars . Paggi, A., Bonato, M., et all. . A&A . 641-62 . 2020 . 2020A&A...641A..62P ,
Instrument EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage 2011-07-11T11:56:04Z/2011-07-12T07:54:42Z
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 2012-07-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-07-28T00:00:00Z, 067287, 17.56_20190403_1200. https://doi.org/10.5270/esa-ac04b57