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.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.other	PURE: 161196763
dc.identifier.other	PURE UUID: 36fce580-08d4-4a01-81e4-d1ed91cc30c3
dc.identifier.other	WOS: 000345826700011
dc.identifier.other	Scopus: 84928200354
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.language.iso	eng
dc.relation.ispartof	Astronomy & Geophysics	en
dc.rights	This 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.subject	Mass	en
dc.title	Quantifying galaxy morphology	en
dc.type	Journal article	en
dc.description.version	Publisher PDF	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