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Conference Paper: New Structure in the Shapley Supercluster

TitleNew Structure in the Shapley Supercluster
Authors
Editors
Editor(s):Colombi, S
Issue Date1998
Citation
Wide Field Surveys in Cosmology: 4th IAP meeting, Paris, France, 26-30 May 1998, p. 392-392 How to Cite?
AbstractWe present new radial velocities for 189 galaxies in a 91 deg^2 region of the Shapley supercluster measured with the FLAIR-II spectrograph on the UK Schmidt Telescope. The data reveal two sheets of galaxies linking the major concentrations of the supercluster. The supercluster is not flattened in Declination as was suggested previously and it may be at least 30% larger than previously thought with a correspondingly larger contribution to the motion of the Local Group.
Persistent Identifierhttp://hdl.handle.net/10722/211283

 

DC FieldValueLanguage
dc.contributor.authorDrinkwater, MJ-
dc.contributor.authorParker, QA-
dc.contributor.authorProust, D-
dc.contributor.authorQuintana, H-
dc.contributor.authorSlezak, E-
dc.contributor.authorMellier, Y-
dc.contributor.authorRaban, B-
dc.contributor.editorColombi, S-
dc.date.accessioned2015-07-08T03:24:08Z-
dc.date.available2015-07-08T03:24:08Z-
dc.date.issued1998-
dc.identifier.citationWide Field Surveys in Cosmology: 4th IAP meeting, Paris, France, 26-30 May 1998, p. 392-392-
dc.identifier.urihttp://hdl.handle.net/10722/211283-
dc.description.abstractWe present new radial velocities for 189 galaxies in a 91 deg^2 region of the Shapley supercluster measured with the FLAIR-II spectrograph on the UK Schmidt Telescope. The data reveal two sheets of galaxies linking the major concentrations of the supercluster. The supercluster is not flattened in Declination as was suggested previously and it may be at least 30% larger than previously thought with a correspondingly larger contribution to the motion of the Local Group.-
dc.languageeng-
dc.relation.ispartofWide Field Surveys in Cosmology-
dc.titleNew Structure in the Shapley Supercluster-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.spage392-
dc.identifier.epage392-

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