A dataset provided by the European Space Agency

Name: The origin of the diffuse radio structure around NGC 5903
Published: 2014-09-03T00:00:00Z

Proposal ID	072227
Title	The origin of the diffuse radio structure around NGC 5903
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722270101
DOI	https://doi.org/10.5270/esa-k3s0jmp
Principal Investigator, PI	Dr Ewan O.Sullivan
Abstract	At present, the only group known to be in the process of converting cold gasinto a hot X-ray emitting intra-group medium and thus starving star-formation inits member galaxies is Stephan.s Quintet. The NGC 5903/ NGC 5898 group may bethe second example. It contains a 100kpc HI filament and a 65kpc diameterdiffuse radio structure which appear to be anti-correlated. A bright ridge inthe radio structure may be a shock driven by a galaxy/HI collision, as inStephan.s Quintet. Alternatively the radio emission may be a remnant of old AGNactivity, but in either case the group should be X-ray luminous. A short (50ks)XMM observation will allow us to discriminate between the two scenarios, andexamine how groups form and maintain their hot intra-group medium.
Publications	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 origin of the X-ray, radio and H I structures in the NGC 5903 galaxy group \|O.Sullivan, Ewan, Kolokythas, Konstantinos, et al. \| MNRAS \| 473-5248 \| 2018 \| 2018MNRAS.473.5248O \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.473.5248O 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	2013-07-30T14:48:05Z/2013-07-31T05:31:25Z
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	2014-09-03T00:00:00Z
Keywords	"starving star formation", "100kpc hi filament", "diffuse radio structure", "bright ridge", "XMM", "hot intra", "xray luminous", "anti correlated", "agn activity", "shock driven", "radio structure", "hi collision", "radio emission", "converting cold gas", "ngc 5898", "ngc 5903", "NGC 5903"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ewan O.Sullivan, 2014, 'The origin of the diffuse radio structure around NGC 5903', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-k3s0jmp