A dataset provided by the European Space Agency

Name 076155
Title A textbook example of ram-pressure stripping in Hydra A
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761550101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761550201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761550301

DOI 10.5270/esa-rjsxz5y
Author Dr Dominique Eckert
Description Ram-pressure stripped tails have been observed in a handful of individual interacting galaxies. In an XMM mosaic program targeting the outskirts of the Hydra A cluster, we discovered a spectacular infalling galaxy group with a very long tail (> 400 kpc long) of hot X-ray emitting gas. This system shows a striking similarity with simulated infalling galaxy groups. It provides a unique opportunity to test our understanding of the ram-pressure stripping process and study the virialization of the infalling gas within the main dark-matter halo. We propose a new 200 ks observation of this accreting substructure with XMM
Publication A textbook example of ram-pressure stripping in the Hydra A-A780 cluster . De Grandi, S., Eckert, D., et all. . A&A . 592-154 . 2016 . 2016A&A...592A.154D ,
The XMM cluster outskirts project (X-COP) . Eckert, D., Ettori, S., et all. . AN . 338-293 . 2017 . 2017AN....338..293E ,
Hydrostatic mass profiles in X-COP galaxy clusters . Ettori, S., Ghirardini, V., et all. . A&A . 621-39 . 2019 . 2019A&A...621A..39E ,
Non-thermal pressure support in X-COP galaxy clusters . Eckert, D., Ghirardini, V., et all. . A&A . 621-40 . 2019 . 2019A&A...621A..40E ,
A New Class of X-Ray Tails of Early-type Galaxies and Subclusters in Galaxy Clusters: Slingshot Tails versus Ram Pressure Stripped Tails . Sheardown, Alex, Fish, Thomas M., et all. . ApJ . 874-112 . 2019 . 2019ApJ...874..112S ,
The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population . Pratt, G. W., Arnaud, M., et all. . SSRv . 215-25 . 2019 . 2019SSRv..215...25P ,
Results from the SuperModel analysis of the X-COP galaxy clusters sample . Fusco-Femiano, Roberto, . MNRAS . 485-1800 . 2019 . 2019MNRAS.485.1800F ,
Polytropic state of the intracluster medium in the X-COP cluster sample . Ghirardini, V., Ettori, S., et all. . A&A . 627-19 . 2019 . 2019A&A...627A..19G ,
Spectral imaging of the thermal Sun...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2015-05-27T05:10:47Z/2015-11-20T02:46:14Z
Version PPS_NOT_AVAILABLE
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 2016-12-29T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016-12-29T23:00:00Z, 076155, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-rjsxz5y