A dataset provided by the European Space Agency

Name: The connection of X-ray tails and HI tails of late-type cluster galaxies
Published: 2011-07-03T00:00:00Z

Proposal ID	065179
Title	The connection of X-ray tails and HI tails of late-type cluster galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651790101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651790201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651790301
DOI	https://doi.org/10.5270/esa-9224b70
Principal Investigator, PI	Dr Ming Sun
Abstract	X-ray tails of late-type cluster galaxies were only detected recently withChandra and XMM. Detailed studies of these systems allow us to better understandram-pressure stripping, galaxy transformation in clusters, mixing of thestripped cold ISM with the hot ICM, r^ant micro-physics and intracluster SF.However, X-ray tails are rare in blind searches, often submerged in strongcluster background. We propose a targeted search for X-ray tails for sixlate-type galaxies with known HI tails in the Virgo cluster. The combination ofVirgo.s proximity, the low cluster background around these galaxies and XMM.spower in the soft X-ray band will put strong constraints on the properties ofX-ray tails even if none are detected, which will also be compared with our simulations.
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 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 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, 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 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 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 composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou, Min-Hua, Gu, Min-Feng, \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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 Gas clumping in the outskirts of the Virgo cluster \|Mirakhor, M. S., Walker, S. A., \| MNRAS \| 506-139 \| 2021 \| 2021MNRAS.506..139M \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506..139M Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster \|Graham, Alister W., Soria, Roberto, et al. \| ApJ \| 923-146 \| 2021 \| 2021ApJ...923..146G \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...923..146G 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 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 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 Variability in a low-mass active galactic nucleus: oscillation or eruption? \|Webbe, Robbie, Young, A. J., \| MNRAS \| 518-3428 \| 2023 \| 2023MNRAS.518.3428W \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.518.3428W 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 Searching for quasi-periodic eruptions using machine learning \|Webbe, Robbie, Young, A. J., \| RASTI \| 2-238 \| 2023 \| 2023RASTI...2..238W \| http://ui.adsabs.harvard.edu/#abs/2023RASTI...2..238W The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2010-06-02T04:55:52Z/2010-06-14T06:49:32Z
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	2011-07-03T00:00:00Z
Keywords	"virgo cluster", "late type galaxy", "XMM", "intracluster sf", "relevant micro physics", "cluster background", "galaxy transformation", "low cluster background", "hi tails", "blind searches", "ram pressure", "targeted search", "stripped cold ism", "hot icm", "soft xray band", "xray tails"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ming Sun, 2011, 'The connection of X-ray tails and HI tails of late-type cluster galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9224b70