A dataset provided by the European Space Agency

Name: Witnessing dramatic galaxy transformation in Abell cluster 1367
Published: 2010-12-04T00:00:00Z

Proposal ID	060220
Title	Witnessing dramatic galaxy transformation in Abell cluster 1367
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602200101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602200201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602200301
DOI	https://doi.org/10.5270/esa-cniqqow
Principal Investigator, PI	Dr Alexis Finoguenov
Abstract	The cluster Abell 1367 provides us with unique opportunities to study theprocesses associated with galaxy transformation in dense environments. Thisdynamically young cluster is currently forming at the intersection of two largescale filaments. Optical observations suggest that it is composed of at leastfour separate dynamical units. Multiple jet-like cometary trails, 150 kpc long,have been discovered in A1367 using H-alpha imaging observations, suggestinggalaxy infall at high-velocity. To interpret these unique data, an understandingof the dynamical state of A1367 is required. We propose to determine the masscomponents of the cluster, their relative motions, and to understand the effectsof mergers on the infalling galaxies by completing the XMM mosaic of this cluster.
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 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 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 HICOSMO - cosmology with a complete sample of galaxy clusters - I. Data analysis sample selection and luminosity-mass scaling relation \|Schellenberger G. Reiprich T. H. \| MNRAS \| 469-3738 \| 2017 \| 2017MNRAS.469.3738S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.469.3738S X-Ray Morphological Analysis of the Planck ESZ Clusters \|Lovisari Lorenzo Forman William R. et al. \| ApJ \| 846-51 \| 2017 \| 2017ApJ...846...51L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...846...51L Correlation between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies \|Bogdan Akos Lovisari Lorenzo et al. \| ApJ \| 852-131 \| 2018 \| 2018ApJ...852..131B \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...852..131B The 3CR Chandra Snapshot Survey: Extragalactic Radio Sources with Redshifts between 1 and 1.5 \|Stuardi C. Missaglia V. et al. \| ApJS \| 235-32 \| 2018 \| 2018ApJS..235...32S \| http://ui.adsabs.harvard.edu/#abs/2018ApJS..235...32S 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 A merger shock in Abell 1367 \|Ge Chong Sun Ming et al. \| MNRAS \| 486-36 \| 2019 \| 2019MNRAS.486L..36G \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486L..36G The TeV-emitting radio galaxy 3C 264. VLBI kinematics and SED modeling \|Boccardi B. Migliori G. et al. \| A&A \| 627-89 \| 2019 \| 2019A&A...627A..89B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...627A..89B Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations \|Bassini L. Rasia E. et al. \| A&A \| 630-144 \| 2019 \| 2019A&A...630A.144B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...630A.144B X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton \|Lovisari Lorenzo Schellenberger Gerrit et al. \| ApJ \| 892-102 \| 2020 \| 2020ApJ...892..102L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892..102L A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O Comparing different mass estimators for a large subsample of the Planck-ESZ clusters \|Lovisari L. Ettori S. et al. \| A&A \| 644-78 \| 2020 \| 2020A&A...644A..78L \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..78L 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 The thermalization of massive galaxy clusters \|Sereno Mauro Lovisari Lorenzo et al. \| MNRAS \| 507-5214 \| 2021 \| 2021MNRAS.507.5214S \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5214S 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 Dark X-Ray Galaxies in the A1367 Galaxy Cluster \|Henriksen Mark J. Dusek Scott \| ApJ \| 917-33 \| 2021 \| 2021ApJ...917L..33H \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...917L..33H An XMM-Newton Early-type Galaxy Atlas \|Islam Nazma Kim Dong-Woo et al. \| ApJS \| 256-22 \| 2021 \| 2021ApJS..256...22I \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..256...22I The BIG X-ray tail \|Ge Chong Sun Ming et al. \| MNRAS \| 508-69 \| 2021 \| 2021MNRAS.508L..69G \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.508L..69G 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 MUSE sneaks a peek at extreme ram-pressure stripping events - V. Towards a complete view of the galaxy cluster A1367 \|Pedrini Alex Fossati Matteo et al. \| MNRAS \| 511-5180 \| 2022 \| 2022MNRAS.511.5180P \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.511.5180P A universal correlation between warm and hot gas in the stripped tails of cluster galaxies \|Sun Ming Ge Chong et al. \| NatAs \| 6-270 \| 2021 \| 2022NatAs...6..270S \| http://ui.adsabs.harvard.edu/#abs/2022NatAs...6..270S High-energy Emission Component Population and Contribution to the Extragalactic Gamma-Ray Background of Gamma-Ray-emitting Radio Galaxies \|Fukazawa Yasushi Matake Hiroto et al. \| ApJ \| 931-138 \| 2022 \| 2022ApJ...931..138F \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...931..138F 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 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 Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters \|Wicker R. Douspis M. et al. \| A&A \| 674-48 \| 2023 \| 2023A&A...674A..48W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A..48W 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	2009-05-27T01:03:09Z/2009-11-25T09:13:27Z
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	2010-12-04T00:00:00Z
Last Update	2025-01-27
Keywords	"separate dynamical units", "infalling galaxy", "galaxy transformation", "abell cluster 1367", "scale filaments", "relative motions", "alpha imaging", "Abell ", "multiple jet", "xmm mosaic", "mass components", "dense environments", "XMM", "cluster abell 1367", "cometary trails", "galaxy infall"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Alexis Finoguenov, 2010, 'Witnessing dramatic galaxy transformation in Abell cluster 1367', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-cniqqow