Locations of peculiar supernovae as a diagnostic of their origins
dc.contributor.author | Yuan, Fang | |
dc.contributor.author | Kobayashi, Chiaki | |
dc.contributor.author | Schmidt, Brian | |
dc.contributor.author | Sim, Stuart A. | |
dc.contributor.author | Podsiadlowski, Ph. | |
dc.contributor.author | Scalzo, Richard | |
dc.date.accessioned | 2015-12-13T22:24:46Z | |
dc.date.issued | 2013 | |
dc.date.updated | 2016-02-24T09:11:44Z | |
dc.description.abstract | We 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.issn | 0035-8711 | |
dc.identifier.uri | http://hdl.handle.net/1885/72895 | |
dc.publisher | Oxford 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.source | Monthly Notices of the Royal Astronomical Society | |
dc.source.uri | https://academic.oup.com/mnras/article/432/2/1680/1031201 | |
dc.subject | Keywords: Galaxies: abundances; Methods: statistical; Supernovae: general | |
dc.title | Locations of peculiar supernovae as a diagnostic of their origins | |
dc.type | Journal article | |
dcterms.accessRights | Open Access | en_AU |
local.bibliographicCitation.issue | 2 | |
local.bibliographicCitation.lastpage | 1686 | |
local.bibliographicCitation.startpage | 1680 | |
local.contributor.affiliation | Yuan, Fang, College of Physical and Mathematical Sciences, The Australian National University | |
local.contributor.affiliation | Kobayashi, Chiaki, University of Hertfordshire | |
local.contributor.affiliation | Schmidt, Brian, College of Physical and Mathematical Sciences, The Australian National University | |
local.contributor.affiliation | Sim, Stuart A, College of Physical and Mathematical Sciences,The Australian National University | |
local.contributor.affiliation | Podsiadlowski, Ph., Oxford University | |
local.contributor.affiliation | Scalzo, Richard, College of Physical and Mathematical Sciences, The Australian National University | |
local.contributor.authoremail | u4981546@anu.edu.au | |
local.contributor.authoruid | Yuan, Fang, u4981546 | |
local.contributor.authoruid | Schmidt, Brian, u9500253 | |
local.contributor.authoruid | Sim, Stuart A, u4967042 | |
local.contributor.authoruid | Scalzo, Richard, u4956999 | |
local.description.notes | Imported from ARIES | |
local.identifier.absfor | 020100 - ASTRONOMICAL AND SPACE SCIENCES | |
local.identifier.ariespublication | f5625xPUB3474 | |
local.identifier.citationvolume | 432 | |
local.identifier.doi | 10.1093/mnras/stt591 | |
local.identifier.essn | 1365-2966 | |
local.identifier.scopusID | 2-s2.0-84878650147 | |
local.identifier.thomsonID | 000319832300065 | |
local.identifier.uidSubmittedBy | f5625 | |
local.type.status | Published Version |
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