A dataset provided by the European Space Agency

Name: Metal Transport and Heating in the Core of the Antlia Cluster
Published: 2011-01-29T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	060489
Title	Metal Transport and Heating in the Core of the Antlia Cluster
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604890101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604890201
DOI	https://doi.org/10.5270/esa-crpidpw
Principal Investigator, PI	Dr Marie Machacek
Abstract	Understanding the transport of energy and metals from central dominant galaxiesin clusters into the intracluster medium (ICM) is vital to any model for theevolution of structure in the Universe. We propose to use a 50ks EPIC MOS+pnobservation of the core (inner 12) of the Antlia Cluster to study the role ofgas motions and turbulent diffusion in the chemical enrichment and heating ofthe ICM in a cluster with a sharply rising abundance profile, but without a coolcore. We will map temperature, density and abundances throughout the Antliacluster core, construct pressure and entropy maps to track gas motions and heatflows, and test models of metal enrichment due to turbulent motions powered byepisodic outbursts from the central galaxys AGN.
Publications	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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Suzaku X-ray Observations of the Nearest Non-Cool Core Cluster Antlia: Dynamically Young but with Remarkably Relaxed Outskirts \|Wong Ka-Wah Irwin Jimmy A. et al. \| ApJ \| 829-49 \| 2016 \| 2016ApJ...829...49W \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829...49W 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 A new clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw H. P. Roberts T. P. et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E 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 impact of precession on the observed population of ULXs \|Khan Norman Middleton Matthew J. et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows R. Comerford Julia M. et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S 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	2010-01-03T02:38:00Z/2010-01-03T20:54:58Z
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	2011-01-29T00:00:00Z
Last Update	2026-07-09
Keywords	"chemical enrichment", "central dominant galaxy", "metal transport", "turbulent diffusion", "episodic outburst", "antlia cluster core", "gas motions", "rising abundance profile", "antlia cluster", "track gas motions", "abundance throughout", "cool core", "EPIC", "test models", "central galaxy", "core inner", "turbulent motions powered", "construct pressure", "metal enrichment", "entropy maps", "intracluster medium icm", "heat flows", "epic mos", "map temperature"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marie Machacek, 2011, 'Metal Transport and Heating in the Core of the Antlia Cluster', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-crpidpw
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.