A dataset provided by the European Space Agency

Name: Tales of tails: the Virgo episodes
Published: 2018-12-27T23:00:00Z

Proposal ID	080258
Title	Tales of tails: the Virgo episodes
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802580101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802580201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802580301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802580401
DOI	https://doi.org/10.5270/esa-tyt42uh
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 better understandingfor ram-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 a sample oflate- type galaxies with known HI tails in the closest cluster, the Virgocluster. The XMM data, in combination with our large CFHT project for a Virgo Hasurvey, will explore the X-ray-Ha correlation in poor environment and put strongconstraints on the properties of X-ray tails even if none are detected.
Publications	A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). IV. A tail of ionised gas in the merger remnant NGC4424 \|Boselli, A., Fossati, M., et al. \| A&A \| 620-164 \| 2018 \| 2018A&A...620A.164B \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A.164B 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 Exploring X-Ray Properties of Low-metallicity Dwarf Galaxies \|Cann, Jenna M., Weaver, Kimberly A., et al. \| ApJ \| 961-178 \| 2024 \| 2024ApJ...961..178C \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..178C 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	2017-06-23T06:19:06Z/2017-12-06T05:10:37Z
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	2018-12-27T23:00:00Z
Keywords	"virgo cluster", "cfht project", "xray ha correlation", "galaxy transformation", "cluster background", "virgo episodes", "intracluster sf", "blind searches", "ram pressure", "hot icm", "late type galaxy", "XMM", "relevant micro physics", "hi tails", "virgo ha survey", "targeted search", "stripped cold ism", "xray tails", "xmm data", "closest cluster"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ming Sun, 2018, 'Tales of tails: the Virgo episodes', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-tyt42uh