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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.identifier161196763
dc.identifier36fce580-08d4-4a01-81e4-d1ed91cc30c3
dc.identifier000345826700011
dc.identifier84928200354
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.urihttps://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.format.extent458339
dc.language.isoeng
dc.relation.ispartofAstronomy & Geophysicsen
dc.subjectMassen
dc.titleQuantifying galaxy morphologyen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1093/astrogeo/atu246
dc.description.statusPeer revieweden


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