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dc.contributor.authorCarpineti, Alfredo
dc.contributor.authorKaviraj, Sugata
dc.contributor.authorHyde, Ashley K.
dc.contributor.authorClements, David L.
dc.contributor.authorSchawinski, Kevin
dc.contributor.authorDarg, Daniel
dc.contributor.authorLintott, Chris J.
dc.date.accessioned2017-07-13T17:02:26Z
dc.date.available2017-07-13T17:02:26Z
dc.date.issued2015-05-13
dc.identifier.citationCarpineti , A , Kaviraj , S , Hyde , A K , Clements , D L , Schawinski , K , Darg , D & Lintott , C J 2015 , ' An infrared study of local galaxy mergers ' , Astronomy & Astrophysics , vol. 577 . https://doi.org/10.1051/0004-6361/201425276
dc.identifier.issn0004-6361
dc.identifier.otherArXiv: http://arxiv.org/abs/1503.07877v1
dc.identifier.otherORCID: /0000-0002-5601-575X/work/77850178
dc.identifier.urihttp://hdl.handle.net/2299/18925
dc.descriptionA. Carpineti, et al., “An infrared study of local galaxy mergers”, Astronomy & Astrophysics, Vol. 577, May 2015. This version of record is available online at: https://doi.org/10.1051/0004-6361/201425276 Reproduced with Permission from Astronomy and Astrophysics, © ESO 2016.
dc.description.abstractWe combine a large, homogeneous sample of $\sim$3000 local mergers with the Imperial IRAS Faint Source Redshift Catalogue (IIFSCz), to perform a blind far-infrared (FIR) study of the local merger population. The IRAS-detected mergers are mostly ($98\%$) spiral-spiral systems, residing in low density environments, a median FIR luminosity of $10^{11} L_\odot$ (which translates to a median star formation rate of around 15$M_\odot yr^{-1}$). The FIR luminosity -- and therefore the star formation rate -- shows little correlation with group richness and scales with the total stellar mass of the system, with little or no dependence on the merger mass ratio. In particular, minor mergers (mass ratios $en
dc.format.extent7
dc.format.extent1950637
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.subjectastro-ph.GA
dc.titleAn infrared study of local galaxy mergersen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1051/0004-6361/201425276
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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