Quantifying galaxy morphology

dc.contributor.author	Pawlik, Milena
dc.date.accessioned	2015-01-05T14:31:02Z
dc.date.available	2015-01-05T14:31:02Z
dc.date.issued	2014-12
dc.identifier	161196763
dc.identifier	36fce580-08d4-4a01-81e4-d1ed91cc30c3
dc.identifier	000345826700011
dc.identifier	84928200354
dc.identifier.citation	Pawlik , M 2014 , ' Quantifying galaxy morphology ' , Astronomy & Geophysics , vol. 55 , no. 6 , pp. 13-16 . https://doi.org/10.1093/astrogeo/atu246	en
dc.identifier.issn	1366-8781
dc.identifier.uri	https://hdl.handle.net/10023/5966
dc.description.abstract	How 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.extent	4
dc.format.extent	458339
dc.language.iso	eng
dc.relation.ispartof	Astronomy & Geophysics	en
dc.subject	Mass	en
dc.title	Quantifying galaxy morphology	en
dc.type	Journal article	en
dc.contributor.institution	University of St Andrews. School of Physics and Astronomy	en
dc.identifier.doi	https://doi.org/10.1093/astrogeo/atu246
dc.description.status	Peer reviewed	en