A dataset provided by the European Space Agency

Name 074493
Title Hunting for large scale cold fronts in sloshing clusters
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744930101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744930201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744930301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744930401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744930501

DOI https://doi.org/10.5270/esa-8lu20dh
Author European Space Agency
Description The cold fronts found at large distances from the center in A2142 and Perseus
changed our understanding of sloshing: not anymore a small disturbance in the
core but a cluster-wide phenomenon reaching half of the virial radius. We
propose offset observations of four known sloshing clusters, showing the most
robust indications of excess surface brightness extending beyond 400 kpc from
the center in ROSAT/PSPC observations. We will search for the presence of large
scale surface brightness discontinuities, contrary to the predictions of
simulations. We will assess if A2142 and Perseus are unique or cold fronts at
large radii are a common feature of sloshing clusters. This program will thus
provide strong constraints to our understanding of sloshing, ICM micro-physics and cluster mergers.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-06-22T22:44:22Z/2015-01-18T04:14:51Z
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 2016-02-12T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016, Hunting For Large Scale Cold Fronts In Sloshing Clusters, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8lu20dh