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Collisional heating as the origin of filament emission in galaxy clusters

dc.contributor.authorFerland G. J.
dc.contributor.authorFabian A. C.
dc.contributor.authorHatch N. A.
dc.contributor.authorJohnstone R. M.
dc.contributor.authorPorter R. L.
dc.contributor.authorvan Hoof P. A. M.
dc.contributor.authorWilliams R. J. R.
dc.date2/2009
dc.date.accessioned2016-04-13T10:04:35Z
dc.date.available2016-04-13T10:04:35Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3741
dc.descriptionhttp://esoads.eso.org/abs/2009MNRAS.392.1475F
dc.languageeng
dc.rightsRestricted Access
dc.titleCollisional heating as the origin of filament emission in galaxy clusters
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleMonthly Notices of the Royal Astronomical Society
dc.source.volume392
dc.source.page1475
Orfeo.peerreviewedYes
dc.identifier.doi10.1111/j.1365-2966.2008.14153.x
dc.identifier.urlhttp://esoads.eso.org/abs/2009MNRAS.392.1475F
dc.source.editorMNRAS


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