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dc.contributor.authorPawlik, Milena
dc.date.accessioned2015-01-05T14:31:02Z
dc.date.available2015-01-05T14:31:02Z
dc.date.issued2014-12
dc.identifier.citationPawlik , M 2014 , ' Quantifying galaxy morphology ' , Astronomy & Geophysics , vol. 55 , no. 6 , pp. 13-16 . https://doi.org/10.1093/astrogeo/atu246en
dc.identifier.issn1366-8781
dc.identifier.otherPURE: 161196763
dc.identifier.otherPURE UUID: 36fce580-08d4-4a01-81e4-d1ed91cc30c3
dc.identifier.otherWOS: 000345826700011
dc.identifier.otherScopus: 84928200354
dc.identifier.urihttp://hdl.handle.net/10023/5966
dc.description.abstractHow do the different shapes of galaxies arise? Milena Pawlik describes work to identify the role of galaxy mergers and starbursts in galactic evolution.
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofAstronomy & Geophysicsen
dc.rightsThis article has been accepted for publication in Astronomy & Geophysics © 2014 Royal Astronomical Society, Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.en
dc.subjectMassen
dc.titleQuantifying galaxy morphologyen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/astrogeo/atu246
dc.description.statusPeer revieweden


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