A dataset provided by the European Space Agency

Name: Understanding the Physics and Dynamics of the NGC4839 Group as it Falls into the
Published: 2013-06-16T00:00:00Z

Proposal ID	069161
Title	Understanding the Physics and Dynamics of the NGC4839 Group as it Falls into the
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691610201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691610301
DOI	https://doi.org/10.5270/esa-qnm9wlf
Principal Investigator, PI	Dr William Forman
Abstract	We propose to complete our investigation of the massive group centered on the cDgalaxy NGC4839, which is falling into the Coma cluster. The completedobservations will allow the physics and dynamics of this merger to be studied inunprecedented detail. Our 112 ks (80 ks plus 40% overhead) XMM-Newtonobservation was badly flared. To complete our program, we request an additional58 ks (which includes 40% overhead). With a complete data set, we will determinethe nature of the shock/sheath region at the interface between the Coma ICM andthe group gas, investigate the newly identified (120x75 kpc) cocoon surroundingNGC4839, and study the 400 kpc ram pressure stripped tail behind NGC4839 todetermine the importance of mixing of cluster gas with stripped group gas.
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 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 The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso, E., Risaliti, G., \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S 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 A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman, Murray, Ward, Charlotte, et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B 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 An XMM-Newton study of active-inactive galaxy pairs \|Guainazzi, Matteo, De Rosa, Alessandra, et al. \| MNRAS \| 504-393 \| 2021 \| 2021MNRAS.504..393G \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.504..393G 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 X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf, J., Nandra, K., et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W 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	2012-06-02T03:09:51Z/2012-06-04T12:59:17Z
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	2013-06-16T00:00:00Z
Keywords	"complete data set", "NGC4839", "XMM", "coma icm", "cd galaxy ngc4839", "XMM-Newton", "sheath region", "badly flared", "coma cluster", "overhead xmm newton", "cluster gas"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr William Forman, 2013, 'Understanding the Physics and Dynamics of the NGC4839 Group as it Falls into the', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qnm9wlf