A dataset provided by the European Space Agency

Name 050626
Title A deep observation of the core and circum-core regions of Abell 496
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506260301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506260401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506260501

DOI 10.5270/esa-m8h84ze
Author Dr Simona Ghizzardi
Description We propose a long, 120 ks, observation of the core and circum-core regions of Abell 496. A detailed observational characterization of cold fronts in cool cores and of circum-core regions are of paramount importance to attempt to constrain heating models from the outside to a degree comparable to that which has already been achieved for models requiring heating from the AGN.
Publication Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton . Matsushita, K., . A&A . 527-134 . 2011 . 2011A&A...527A.134M ,
Gas sloshing, cold fronts, Kelvin-Helmholtz instabilities and the merger history of the cluster of galaxies Abell 496 . Roediger, E., Lovisari, L., et all. . MNRAS . 420-3632 . 2012 . 2012MNRAS.420.3632R ,
Cold fronts in galaxy clusters . Ghizzardi, S., Rossetti, M., . A&A . 516-32 . 2010 . 2010A&A...516A..32G ,
Inhomogeneous metal distribution in the intracluster medium . Lovisari, L., Schindler, S., . A&A . 528-60 . 2011 . 2011A&A...528A..60L ,
Constraints on turbulent velocity broadening for a sample of clusters, groups and elliptical galaxies using XMM-Newton . Sanders, J. S., Fabian, A. C., . MNRAS . 410-1797 . 2011 . 2011MNRAS.410.1797S ,
Revealing O VII from stacked X-ray grating spectra of clusters, groups and elliptical galaxies . Sanders, J. S., Fabian, A. C., . MNRAS . 412-35 . 2011 . 2011MNRAS.412L..35S ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
On the Origin of the Extended Halpha Filaments in Cooling Flow Clusters . McDonald, Michael, Veilleux, Sylvain, et all. . ApJ . 721-1262 . 2010 . 2010ApJ...721.1262M ,
Exospheric solar wind charge exchange a...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-08-11T14:17:40Z/2008-02-19T15:24:47Z
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 2009-04-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-04-02T00:00:00Z, 050626, 17.56_20190403_1200. https://doi.org/10.5270/esa-m8h84ze