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Implications of coronal line emission in NGC 4696*

dc.contributor.authorChatzikos M.
dc.contributor.authorWilliams R. J. R.
dc.contributor.authorFerland G. J.
dc.contributor.authorCanning R. E. A.
dc.contributor.authorFabian A. C.
dc.contributor.authorSanders J. S.
dc.contributor.authorvan Hoof P. A. M.
dc.contributor.authorJohnstone R. M.
dc.contributor.authorLykins M.
dc.contributor.authorPorter R. L.
dc.date1/2015
dc.date.accessioned2016-04-13T10:08:13Z
dc.date.available2016-04-13T10:08:13Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3947
dc.descriptionhttp://esoads.eso.org/abs/2015MNRAS.446.1234C
dc.languageeng
dc.rightsRestricted Access
dc.titleImplications of coronal line emission in NGC 4696<SUP>*</SUP>
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleMonthly Notices of the Royal Astronomical Society
dc.source.volume446
dc.source.page1234
Orfeo.peerreviewedYes
dc.identifier.doi10.1093/mnras/stu2173
dc.identifier.urlhttp://esoads.eso.org/abs/2015MNRAS.446.1234C
dc.source.editorOUP


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