Kinetic Sunyaev-Zeldovich effect from galaxy cluster rotation

Publication:
Kinetic Sunyaev-Zeldovich effect from galaxy cluster rotation

dc.bibliographiccitation.firstpage	419
dc.bibliographiccitation.issue	2
dc.bibliographiccitation.journal	Astronomy and Astrophysics
dc.bibliographiccitation.lastpage	427
dc.bibliographiccitation.volume	396
dc.contributor.author	Chluba, J.
dc.contributor.author	Mannheim, K.
dc.date.accessioned	2018-11-07T09:43:15Z
dc.date.available	2018-11-07T09:43:15Z
dc.date.issued	2002
dc.description.abstract	We show how the temperature and the polarization of the cosmic microwave background are affected by bulk rotation of clusters of galaxies owing to the kinetic Sunyaev-Zeldovich effect. The main effects of rotation are (i) a shift of the position of the peak of the temperature fluctuation relative to the center of the cluster by a few percent of the core radius and (ii) a tilt of the direction of the plane of linear polarization by several degrees.
dc.identifier.doi	10.1051/0004-6361:20021429
dc.identifier.isi	000179574300008
dc.identifier.purl	https://resolver.sub.uni-goettingen.de/purl?gs-1/9786
dc.identifier.uri	https://resolver.sub.uni-goettingen.de/purl?gro-2/34138
dc.item.fulltext	With Fulltext
dc.notes.intern	Merged from goescholar
dc.notes.status	zu prüfen
dc.notes.submitter	Najko
dc.publisher	E D P Sciences
dc.relation.issn	0004-6361
dc.relation.orgunit	Fakultät für Physik
dc.title	Kinetic Sunyaev-Zeldovich effect from galaxy cluster rotation
dc.type	journal_article
dc.type.internalPublication	yes
dc.type.peerReviewed	yes
dc.type.status	published
dc.type.version	published_version
dspace.entity.type	Publication

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