A dataset provided by the European Space Agency

Name: Jets at work: 3C 386 comma driven outflow or runaway feedbackquestionMark
Published: 2014-10-01T00:00:00Z

Proposal ID	072243
Title	Jets at work: 3C 386, driven outflow or runaway feedback?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722430101
DOI	https://doi.org/10.5270/esa-d3esnzj
Principal Investigator, PI	Prof Diana Worrall
Abstract	A key ingredient of structure evolution at late times is the accretion energythat is redistributed into the external medium through radio sources, via poorlyunderstood energy-exchange mechanisms. Many sources in group environmentsdisplay prominent belt-like X-ray structures that are associated with thecentral narrowing of radio sources between their X-ray-filled lobes. The beltsare not like cluster cavity features, and could either be a driven outflow ofcooler gas from the centre, and a potential barrier to feedback, or displacedgas associated with fuelling the AGN, potentially causing runaway feedback. Wepropose to test which is the case in 3C 386, our best example of a nearbydouble-lobed radio source with a prominent X-ray belt in a poor environment.
Publications	Buoyancy-driven inflow to a relic cold core: the gas belt in radio galaxy 3C 386 \|Duffy, R. T., Worrall, D. M., et al. \| MNRAS \| 459-4508 \| 2016 \| 2016MNRAS.459.4508D \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.459.4508D 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 The 3CR Chandra Snapshot Survey: Extragalactic Radio Sources with Redshifts between 1 and 1.5 \|Stuardi, C., Missaglia, V., et al. \| ApJS \| 235-32 \| 2018 \| 2018ApJS..235...32S \| http://ui.adsabs.harvard.edu/#abs/2018ApJS..235...32S 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-09-11T18:50:28Z/2013-09-12T20:23:48Z
Version	17.56_20190403_1200
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	2014-10-01T00:00:00Z
Keywords	"xray filled lobes", "displaced gas", "central narrowing", "potential barrier", "driven outflow", "radio sources", "prominent xray belt", "cluster cavity", "xray structures", "external medium", "cooler gas", "energy exchange mechanisms", "key ingredient", "structure evolution", "3c 386", "via poorly", "runaway feedback ?.", "accretion energy"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Diana Worrall, 2014, 'Jets at work: 3C 386 comma driven outflow or runaway feedbackquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-d3esnzj