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The origin of Segue 1

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dc.contributor.authorNiederste-Ostholt, M.
dc.contributor.authorBelokurov, Vasily
dc.contributor.authorEvans, N W
dc.contributor.authorGilmore, Gerard
dc.contributor.authorWyse, Rosemary F G
dc.contributor.authorNorris, John
dc.date.accessioned2015-12-08T22:16:39Z
dc.date.issued2009
dc.date.updated2016-02-24T09:55:18Z
dc.description.abstractWe apply the optimal filter technique to Sloan Digital Sky Survey photometry around Segue 1 and find that the outer parts of the cluster are distorted. There is strong evidence for ∼1° elongations of extra-tidal stars, extending both eastwards and sout
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/30773
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Galaxies: kinematics and dynamics; Globular clusters: individual: Segue 1
dc.titleThe origin of Segue 1
dc.typeJournal article
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage1781
local.bibliographicCitation.startpage1771
local.contributor.affiliationNiederste-Ostholt, M., Institute of Astronomy, UK
local.contributor.affiliationBelokurov, Vasily, University of Cambridge
local.contributor.affiliationEvans, N W, University of Cambridge
local.contributor.affiliationGilmore, Gerard, University of Cambridge
local.contributor.affiliationWyse, Rosemary F G, Johns Hopkins University
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidNorris, John, u7401084
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationu3356449xPUB77
local.identifier.citationvolume398
local.identifier.doi10.1111/j.1365-2966.2009.15287.x
local.identifier.scopusID2-s2.0-70349216830
local.identifier.thomsonID000269906400014
local.type.statusPublished Version

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