A dataset provided by the European Space Agency

Name: The nature of the filaments in the giant lobes of Centaurus A
Published: 2015-03-04T23:00:00Z

Proposal ID	072462
Title	The nature of the filaments in the giant lobes of Centaurus A
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724620101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724620201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724620301
DOI	https://doi.org/10.5270/esa-aopckvx
Principal Investigator, PI	Ms Sarka Wykes
Abstract	Recent high-resolution radio continuum images of the entirety of the nearestradio galaxy Centaurus A using ATCA and Parkes have revealed intricate radiostructure in its southern giant lobe. Two prominent filaments, named the vertexand the vortex, plausibly originating from an enhanced jet activity of theparent AGN, are the brightest (in flux) filamentary structures known in anyradio galaxy. We propose deep XMM-Newton observations of the brighter of these,the vertex, that will allow us to constrain the physical properties and theorigin of the filaments, and the distribution of internal energy within thelobes, and that may give us a more complete picture of localised particleacceleration in the large-scale lobes.
Publications	Centaurus A: constraints on the nature of the giant lobe filaments from XMM-Newton observations \|Wykes, Sarka, Hardcastle, Martin J., \| MNRAS \| 454-3277 \| 2015 \| 2015MNRAS.454.3277W \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.454.3277W 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 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	2014-01-07T10:53:19Z/2014-02-15T22:37:30Z
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	2015-03-04T23:00:00Z
Keywords	"deep xmm newton", "internal energy", "XMM", "giant lobes", "flux filamentary structures", "southern giant lobe", "prominent filaments", "scale lobes", "localised particle acceleration", "intricate radio structure", "physical properties", "XMM-Newton", "parent agn", "complete picture", "enhanced jet activity", "radiogalaxy centaurus"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Sarka Wykes, 2015, 'The nature of the filaments in the giant lobes of Centaurus A', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-aopckvx