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dc.contributor.authorMagdalenić J.
dc.contributor.authorMarqué C.
dc.contributor.authorZhukov A. N.
dc.contributor.authorVršnak B.
dc.contributor.authorŽic T.
dc.date7/2010
dc.date.accessioned2016-04-13T10:04:31Z
dc.date.available2016-04-13T10:04:31Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3645
dc.descriptionhttp://esoads.eso.org/abs/2010ApJ...718..266M
dc.languageeng
dc.rightsRestricted Access
dc.titleOrigin of Coronal Shock Waves Associated with Slow Coronal Mass Ejections
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleThe Astrophysical Journal
dc.source.volume718
dc.source.page266
Orfeo.peerreviewedYes
dc.identifier.doi10.1088/0004-637X/718/1/266
dc.identifier.urlhttp://esoads.eso.org/abs/2010ApJ...718..266M
dc.source.editorIOP


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