A dataset provided by the European Space Agency

Name: Interaction of a massive cluster system with the embedding cosmic filament
Published: 2018-07-26T22:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	080355
Title	Interaction of a massive cluster system with the embedding cosmic filament
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803550101
DOI	https://doi.org/10.5270/esa-rynuk1f
Principal Investigator, PI	Dr Gayoung Chon
Abstract	The galaxy cluster system RXCJ0225.9-4154 with the two sub-clusters A3016 andA3017 embedded in a large-scale structure filament shows very excitingsignatures of filamentary accretion. The filament can be traced over 6 Mpc bygalaxies and over more than half of its length we observe it in X-ray emission.The main cluster shows indications of shocks most probably from a recent mergeralong the filament axis. The filament between the two sub-clusters seems to beheated by the accretion shocks of the clusters. To study this rich accretionscenario better than with the available Chandra exposure, we propose anXMM-Newton observation of the system for 70 ks.
Publications	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 Dynamical state of galaxy clusters evaluated from X-ray images \|Yuan Z. S. Han J. L. \| MNRAS \| 513-3013 \| 2022 \| 2022MNRAS.513.3013Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.3013Y 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 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	2017-06-25T11:51:53Z/2017-06-26T10:20:13Z
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	2018-07-26T22:00:00Z
Last Update	2026-07-09
Keywords	"XMM-Newton", "scale structure filament", "chandra exposure", "main cluster", "rich accretion scenario", "accretion shoc", "embedding cosmic filament", "sub clusters a3016", "XMM", "sub clusters", "filamentary accretion", "xmm newton", "xray emission", "a3017 embedded", "filament axis", "exciting signatures", "massive cluster system"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gayoung Chon, 2018, 'Interaction of a massive cluster system with the embedding cosmic filament', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-rynuk1f
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.