Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/9182
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dc.contributor.authorProust, D.cat
dc.contributor.authorMazure, Alaincat
dc.contributor.authorTalavera, A.cat
dc.contributor.authorSalvador Solé, Eduardcat
dc.contributor.authorCapelato, H. V.cat
dc.date.accessioned2009-08-24T08:07:10Z-
dc.date.available2009-08-24T08:07:10Z-
dc.date.issued1987cat
dc.identifier.issn0365-0138cat
dc.identifier.urihttp://hdl.handle.net/2445/9182-
dc.description.abstractRedshifts for 100 galaxies in 10 clusters of galaxies are presented based on data obtained between March 1984 and March 1985 from Calar Alto, La Palma, and ESO, and on data from Mauna Kea. Data for individual galaxies are given, and the accuracy of the velocities of the four instruments is discussed. Comparison with published data shows the present velocities to be shifted by + 4.0 km/s on average, with a standard deviation in the difference of 89.7 km/s, consistent with the rms of redshift measurements which range from 50-100 km/s.eng
dc.format.extent5 p.cat
dc.format.mimetypeapplication/pdfeng
dc.language.isoengeng
dc.publisherEDP Sciencescat
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per NASA Astrophysics Data System http://adsabs.harvard.edu/cat
dc.relation.ispartofAstronomy and Astrophysics Supplement Series, 1987, vol. 67, núm. 1, p. 57-61.cat
dc.rights(c) The European Southern Observatory, 1987cat
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationGalàxiescat
dc.subject.classificationClústerscat
dc.subject.classificationAstrofísicacat
dc.subject.otherRedshifts of galaxieseng
dc.subject.otherClusters of galaxieseng
dc.titleNew measurements of radial velocities in clusters of galaxieseng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec35559cat
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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