Investigating the origin of cyclical wind variability in hot massive stars - II. Hydrodynamical simulations of corotating interaction regions using realistic spot parameters for the O giant xi Persei

dc.contributor.author	Kee, Nathaniel Dylan
dc.date.accessioned	2019-04-29T07:58:35Z
dc.date.available	2019-04-29T07:58:35Z
dc.date.issued	2017
dc.identifier.issn	1365-2966
dc.identifier.uri	http://hdl.handle.net/10900/88143
dc.language.iso	en	de_DE
dc.publisher	Oxford Univ Press	de_DE
dc.relation.uri	http://dx.doi.org/10.1093/mnras/stx1478	de_DE
dc.rights	info:eu-repo/semantics/closedAccess
dc.subject.ddc	520	de_DE
dc.subject.ddc	530	de_DE
dc.title	Investigating the origin of cyclical wind variability in hot massive stars - II. Hydrodynamical simulations of corotating interaction regions using realistic spot parameters for the O giant xi Persei	de_DE
dc.type	Article	de_DE
utue.quellen.id	20190131163842_01559
utue.publikation.seiten	3672-3684	de_DE
utue.personen.roh	David-Uraz, A.
utue.personen.roh	Owocki, S. P.
utue.personen.roh	Wade, G. A.
utue.personen.roh	Sundqvist, J. O.
utue.personen.roh	Kee, N. D.
dcterms.isPartOf.ZSTitelID	Monthly Notices of The Royal Astronomical Society	de_DE
dcterms.isPartOf.ZS-Issue	3	de_DE
dcterms.isPartOf.ZS-Volume	470	de_DE
utue.fakultaet	07 Mathematisch-Naturwissenschaftliche Fakultät	de_DE