A dataset provided by the European Space Agency

Name: Understanding the Physics and Dynamics of NGC4839 Group as It Falls into Coma
Published: 2012-01-18T00:00:00Z

Proposal ID	065231
Title	Understanding the Physics and Dynamics of NGC4839 Group as It Falls into Coma
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652310201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652310301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652310401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652310501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652310601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652310701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652310801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652310901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652311001
DOI	https://doi.org/10.5270/esa-kh5i82u
Principal Investigator, PI	Dr William Forman
Abstract	An 80 ks XMM-Newton observation, along with a 40 ks Chandra pointing, of themassive group centered on the cD galaxy NGC4839, which is falling into the Comacluster core, will provide the first excellent map of the merging subcluster andallow the physics and dynamics of this merger to be studied in unprecedenteddetail. The proposed observations will determine the nature of the hot core inNGC4839, including the AGN outburst power. We also will measure the total (3D)velocity of the merging group and the properties of the shock/sheath region atthe interface between the Coma ICM and the group gas, and finally, will computethe gas mass in NGC4839.s 400 kpc tail to determine the importance of mixing ofcluster gas with the stripped group gas.
Publications	Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state \|Castro, M., D.Amico, F., et al. \| A&A \| 569-82 \| 2014 \| 2014A&A...569A..82C \| http://ui.adsabs.harvard.edu/#abs/2014A&A...569A..82C 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 XMM-Newton publication statistics \|Ness, J.-U., Parmar, A. N., et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V 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 sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 \|Pons, E., Watson, M. G., \| A&A \| 594-72 \| 2016 \| 2016A&A...594A..72P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..72P A Catalog Sample of Low-mass Galaxies Observed in X-Rays with Central Candidate Black Holes \|Nucita, A. A., Manni, L., et al. \| ApJ \| 837-66 \| 2017 \| 2017ApJ...837...66N \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...837...66N A New Class of X-Ray Tails of Early-type Galaxies and Subclusters in Galaxy Clusters: Slingshot Tails versus Ram Pressure Stripped Tails \|Sheardown, Alex, Fish, Thomas M., et al. \| ApJ \| 874-112 \| 2019 \| 2019ApJ...874..112S \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...874..112S Close-up view of an ongoing merger between the NGC 4839 group and the Coma cluster - a post-merger scenario \|Lyskova, N., Churazov, E., et al. \| MNRAS \| 485-2922 \| 2019 \| 2019MNRAS.485.2922L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.2922L Measuring bulk flows of the intracluster medium in the Perseus and Coma galaxy clusters using XMM-Newton \|Sanders, J. S., Dennerl, K., et al. \| A&A \| 633-42 \| 2020 \| 2020A&A...633A..42S \| http://ui.adsabs.harvard.edu/#abs/2020A&A...633A..42S Ram pressure stripping candidates in the coma cluster: evidence for enhanced star formation \|Roberts, Ian D., Parker, Laura C., \| MNRAS \| 495-554 \| 2020 \| 2020MNRAS.495..554R \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.495..554R A complete view of the outskirts of the Coma cluster \|Mirakhor, M. S., Walker, S. A., \| MNRAS \| 497-3204 \| 2020 \| 2020MNRAS.497.3204M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3204M Probing ultradiffuse galaxies out to the virial radius of the Coma cluster with XMM-Newton \|Mirakhor, M. S., Walker, S. A., \| MNRAS \| 503-679 \| 2021 \| 2021MNRAS.503..679M \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503..679M 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 Local Active Galactic Nuclei with Large Broad-H\\u03b1 Variability Reside in Red Galaxies \|Liu, Wen-Juan, Lira, Paulina, et al. \| ApJ \| 915-63 \| 2021 \| 2021ApJ...915...63L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...915...63L The Coma Cluster at LOFAR Frequencies. II. The Halo, Relic, and a New Accretion Relic \|Bonafede, A., Brunetti, G., et al. \| ApJ \| 933-218 \| 2022 \| 2022ApJ...933..218B \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...933..218B High-resolution, High-sensitivity, Low-frequency uGMRT View of Coma Cluster of Galaxies \|Lal, D. V., Lyskova, N., et al. \| ApJ \| 934-170 \| 2022 \| 2022ApJ...934..170L \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...934..170L ELUCID. VII. Using Constrained Hydro Simulations to Explore the Gas Component of the Cosmic Web \|Li, Renjie, Wang, Huiyuan, et al. \| ApJ \| 936-11 \| 2022 \| 2022ApJ...936...11L \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...936...11L Baryon cycles in the biggest galaxies \|Donahue, Megan, Voit, G. Mark, \| PhR \| 973-1 \| 2022 \| 2022PhR...973....1D \| http://ui.adsabs.harvard.edu/#abs/2022PhR...973....1D A deep dive: Chandra observations of the NGC 4839 group falling into the Coma cluster \|Mirakhor, M. S., Walker, S. A., \| MNRAS \| 522-2105 \| 2023 \| 2023MNRAS.522.2105M \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.522.2105M A Deep Redshift Survey of the Perseus Cluster (A426): Spatial Distribution and Kinematics of Galaxies \|Kang, Wooseok, Hwang, Ho Seong, et al. \| ApJS \| 272-22 \| 2024 \| 2024ApJS..272...22K \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..272...22K 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	2010-06-16T11:44:20Z/2010-12-11T06:41:06Z
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	2012-01-18T00:00:00Z
Keywords	"agn outburst power", "NGC4839", "XMM", "merging subcluster", "total 3d velocity", "coma cluster core", "coma icm", "hot core", "gas mass", "cd galaxy ngc4839", "XMM-Newton", "sheath region", "cluster gas", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr William Forman, 2012, 'Understanding the Physics and Dynamics of NGC4839 Group as It Falls into Coma', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kh5i82u