A dataset provided by the European Space Agency

Name 065179
Title The connection of X-ray tails and HI tails of late-type cluster galaxies
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651790101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651790201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651790301

DOI 10.5270/esa-9224b70
Author Dr Ming Sun
Description X-ray tails of late-type cluster galaxies were only detected recently with Chandra and XMM. Detailed studies of these systems allow us to better understand ram-pressure stripping, galaxy transformation in clusters, mixing of the stripped 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 strong cluster background. We propose a targeted search for X-ray tails for six late-type galaxies with known HI tails in the Virgo cluster. The combination of Virgo.s proximity, the low cluster background around these galaxies and XMM.s power in the soft X-ray band will put strong constraints on the properties of X-ray tails even if none are detected, which will also be compared with our simulations.
Publication 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 ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster . Planck Collaboration, Ade, P. A. R., et all. . A&A . 596-101 . 2016 . 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 ,
A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies . Earnshaw, H. P., Roberts, T. P., et all. . MNRAS . 483-5554 . 2019 . 2019MNRAS.483.5554E ,
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies . Ojha, Vineet, Chand, Hum, et all. . ApJ . 896-95 . 2020 . 2020ApJ...896...95O ,
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-07-03T00:00:00Z, 065179, 17.56_20190403_1200. https://doi.org/10.5270/esa-9224b70