Locations of peculiar supernovae as a diagnostic of their origins

dc.contributor.authorYuan, Fang
dc.contributor.authorKobayashi, Chiaki
dc.contributor.authorSchmidt, Brian
dc.contributor.authorSim, Stuart A.
dc.contributor.authorPodsiadlowski, Ph.
dc.contributor.authorScalzo, Richard
dc.date.accessioned2015-12-13T22:24:46Z
dc.date.issued2013
dc.date.updated2016-02-24T09:11:44Z
dc.description.abstractWe put constraints on the properties of the progenitors of peculiar calcium-rich transients using the distribution of locations within their host galaxies. We confirm that this class of transients do not follow the galaxy stellar mass profile and are more
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/72895
dc.publisherOxford University Press
dc.rights© 2013 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. This article has been accepted for publication in Monthly Notices of the Royal Astronomical Sociey © 2013 Fang Yuan, Chiaki Kobayashi, Brian P. Schmidt, Philipp Podsiadlowski, Stuart A. Sim, Richard A. Scalzo. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. https://academic.oup.com/journals/pages/ access_purchase/rights_and_permissions/self_archiving_policy_p (Publisher journal website as of 3/10/2018)http://www.sherpa.ac.uk/romeo/issn/0035-8711/ Author can archive publisher's version/PDF. Publisher's version/PDF on Institutional repositories or Central repositories, with all rights reserved (Sherpa/Romeo as of 3/10/2018).en_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.source.urihttps://academic.oup.com/mnras/article/432/2/1680/1031201
dc.subjectKeywords: Galaxies: abundances; Methods: statistical; Supernovae: general
dc.titleLocations of peculiar supernovae as a diagnostic of their origins
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage1686
local.bibliographicCitation.startpage1680
local.contributor.affiliationYuan, Fang, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationKobayashi, Chiaki, University of Hertfordshire
local.contributor.affiliationSchmidt, Brian, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationSim, Stuart A, College of Physical and Mathematical Sciences,The Australian National University
local.contributor.affiliationPodsiadlowski, Ph., Oxford University
local.contributor.affiliationScalzo, Richard, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.authoremailu4981546@anu.edu.au
local.contributor.authoruidYuan, Fang, u4981546
local.contributor.authoruidSchmidt, Brian, u9500253
local.contributor.authoruidSim, Stuart A, u4967042
local.contributor.authoruidScalzo, Richard, u4956999
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB3474
local.identifier.citationvolume432
local.identifier.doi10.1093/mnras/stt591
local.identifier.essn1365-2966
local.identifier.scopusID2-s2.0-84878650147
local.identifier.thomsonID000319832300065
local.identifier.uidSubmittedByf5625
local.type.statusPublished Version

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