The ejected mass distribution of Type Ia supernovae: a significant rate of non-Chandrasekhar-mass progenitors
dc.contributor.author | Scalzo, R. A. | |
dc.contributor.author | Ruiter, A. J. | |
dc.contributor.author | Sim, S. A. | |
dc.date.accessioned | 2015-05-11T01:57:05Z | |
dc.date.available | 2015-05-11T01:57:05Z | |
dc.date.issued | 2014-10-20 | |
dc.date.updated | 2015-12-10T10:39:41Z | |
dc.description.abstract | The ejected mass distribution of Type Ia supernovae (SNe Ia) directly probes progenitor evolutionary history and explosion mechanisms, with implications for their use as cosmological probes. Although the Chandrasekhar mass is a natural mass scale for the | |
dc.description.sponsorship | Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-Sky Astrophysics (CAASTRO), through project number CE110001020. RS and AJR acknowledge support from ARC Laureate Grant FL0992131. | en_AU |
dc.identifier.issn | 0035-8711 | en_AU |
dc.identifier.uri | http://hdl.handle.net/1885/13424 | |
dc.publisher | Oxford University Press | |
dc.relation | http://purl.org/au-research/grants/arc/CE110001020 | |
dc.relation | http://purl.org/au-research/grants/arc/FL0992131 | |
dc.rights | http://www.sherpa.ac.uk/romeo/issn/0035-8711/..."Author's Post-print and Publisher's version/PDF on Institutional repositories or Central repositories, Set phrase to accompany archived copy (see policy)" from SHERPA/RoMEO site (as at 11/05/15) This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | |
dc.source | Monthly Notices of the Royal Astronomical Society | |
dc.subject | methods: statistical | |
dc.subject | supernovae: general | |
dc.subject | white dwarfs | |
dc.subject | dark energy | |
dc.title | The ejected mass distribution of Type Ia supernovae: a significant rate of non-Chandrasekhar-mass progenitors | |
dc.type | Journal article | |
dcterms.dateAccepted | 2014-09-01 | |
local.bibliographicCitation.issue | 3 | en_AU |
local.bibliographicCitation.lastpage | 2544 | en_AU |
local.bibliographicCitation.startpage | 2535 | en_AU |
local.contributor.affiliation | Scalzo, R. A., Research School of Astronomy and Astrophysics, The Australian National University | en_AU |
local.contributor.affiliation | Ruiter, A. J., Research School of Astronomy and Astrophysics, The Australian National University | en_AU |
local.contributor.authoremail | richard.scalzo@anu.edu.au | en_AU |
local.contributor.authoruid | u4956999 | en_AU |
local.identifier.absfor | 020100 - ASTRONOMICAL AND SPACE SCIENCES | |
local.identifier.absseo | 970102 - Expanding Knowledge in the Physical Sciences | |
local.identifier.ariespublication | a383154xPUB1372 | |
local.identifier.citationvolume | 445 | en_AU |
local.identifier.doi | 10.1093/mnras/stu1808 | en_AU |
local.identifier.scopusID | 2-s2.0-84924546675 | |
local.identifier.thomsonID | 000346962900031 | |
local.identifier.uidSubmittedBy | u1005913 | en_AU |
local.publisher.url | http://www.oxfordjournals.org/en/ | en_AU |
local.type.status | Published Version | en_AU |
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