A dataset provided by the European Space Agency

Name: Mach cones around Virgo Cluster spiral galaxies
Published: 2012-07-01T00:00:00Z

Proposal ID	067514
Title	Mach cones around Virgo Cluster spiral galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675140101
DOI	https://doi.org/10.5270/esa-lo6n5cj
Principal Investigator, PI	Dr Marek Wezgowiec
Abstract	The detailed comparison between observations and simulations of ram pressurestripped spiral galaxies in the Virgo cluster has led to a three dimensionalview of the galaxy orbits within the hot intracluster medium. The 3D velocitiesand Mach numbers derived from these simulations can be used to derive simpleMach cone geometries. We see indications of these Mach cones in the large-scaleX-ray emission of existing XMM-Newton data. However, the data are not deepenough to establish a clear cone structure. Therefore, we propose highsensitivity X-ray observations of selected Virgo Cluster spiral galaxies. Theobservations of NGC,4388 were approved in AO9 with a C-priority. However, thishas not been scheduled yet and there is no guarantee it will be done.
Publications	Insight into Active Galactic Nucleus and Host Galaxy Co-evolution from Hard X-Ray Emission \|Wang J. Zhou X. L. \| ApJ \| 768-176 \| 2013 \| 2013ApJ...768..176W \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...768..176W Multi-wavelength Studies of Spectacular Ram Pressure Stripping of a Galaxy: Discovery of an X-Ray Absorption Feature \|Gu Liyi Yagi Masafumi et al. \| ApJ \| 777-36 \| 2013 \| 2013ApJ...777L..36G \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...777L..36G Synapses of active galactic nuclei:. Comparing X-ray and optical classifications using artificial neural networks \|Gonzalez-Martin O. Diaz-Gonzalez D. et al. \| A&A \| 567-92 \| 2014 \| 2014A&A...567A..92G \| http://ui.adsabs.harvard.edu/#abs/2014A&A...567A..92G Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state \|Castro M. DAmico 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 X-ray spectral parameters for a sample of 95 active galactic nuclei \|Vasylenko A. A. Zhdanov V. I. \| Ap&SS \| 360-71 \| 2015 \| 2015Ap&SS.360...71V \| http://ui.adsabs.harvard.edu/#abs/2015Ap&SS.360...71V 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 A comprehensive analysis of the hard X-ray spectra of bright Seyfert galaxies \|Lubinski P. Beckmann V. et al. \| MNRAS \| 458-2454 \| 2016 \| 2016MNRAS.458.2454L \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.458.2454L 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 Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster \|Planck Collaboration Ade P. A. R. et al. \| A&A \| 596-101 \| 2016 \| 2016A&A...596A.101P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...596A.101P 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 The coronal temperature of NGC 4388 and NGC 2110 measured with INTEGRAL \|Ursini F. Bassani L. et al. \| A&A \| 629-54 \| 2019 \| 2019A&A...629A..54U \| http://ui.adsabs.harvard.edu/#abs/2019A&A...629A..54U A Hard Look at Local Optically Selected Obscured Seyfert Galaxies \|Kammoun E. S. Miller J. M. et al. \| ApJ \| 901-161 \| 2020 \| 2020ApJ...901..161K \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...901..161K 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 Chemical enrichment of the ICM within the virgo cluster - I. Radial profiles \|Gatuzz Efrain Sanders J. S. et al. \| MNRAS \| 520-4793 \| 2023 \| 2023MNRAS.520.4793G \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.520.4793G Hydrogen column density variability in a sample of local Compton-thin AGN \|Torres-Albu00e0 N. Marchesi S. et al. \| A&A \| 678-154 \| 2023 \| 2023A&A...678A.154T \| http://ui.adsabs.harvard.edu/#abs/2023A&A...678A.154T A Simple Method for Predicting N H Variability in Active Galactic Nuclei \|Cox Isaiah S. Torres-Albu00e0 Nu00faria et al. \| ApJ \| 958-155 \| 2023 \| 2023ApJ...958..155C \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...958..155C 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	2011-06-17T23:22:39Z/2011-06-18T16:25:51Z
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	2012-07-01T00:00:00Z
Last Update	2025-01-27
Keywords	"cone structure", "galaxy orbits", "scale xray emission", "XMM-Newton", "virgo cluster", "mach cones", "sensitivity xray", "NGC", "hot intracluster medium", "3d velocities", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marek Wezgowiec, 2012, 'Mach cones around Virgo Cluster spiral galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-lo6n5cj