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Subaru High-Resolution Spectroscopy of Star G in the Tycho Supernova Remnant

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dc.contributor.authorKerzendorf, Wolfgang
dc.contributor.authorSchmidt, Brian
dc.contributor.authorAsplund, Martin
dc.contributor.authorNomoto, Ken'ichi
dc.contributor.authorPodsiadlowski, Ph.
dc.contributor.authorFrebel, Anna
dc.contributor.authorFesen, Robert A
dc.contributor.authorYong, David
dc.date.accessioned2015-12-08T22:19:22Z
dc.date.issued2009
dc.date.updated2016-02-24T09:55:23Z
dc.description.abstractIt is widely believed that Type Ia supernovae (SNe Ia) originate in binary systems where a white dwarf accretes material from a companion star until its mass approaches the Chandrasekhar mass and carbon is ignited in the white dwarf's core. This scenario
dc.description.sponsorshipW.E.K., B.P.S., and M.A. are supported by the Australian Research Council (grant DP0559024, FF0561481). This paper was conceived as part of the Tokyo Think Tank collaboration, and was supported in part by the National Science Foundation under grant PHY05-51164. This work was supported in part by World Premier International Research Center Initiative (WPI Program), MEXT, Japan, and by the Grant-in-Aid for Scientific Research of the Japan Society for the Promotion of Science (18104003, 18540231, 20540226) and MEXT (19047004, 20040004).
dc.format8 pages
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/31537
dc.provenancehttp://www.sherpa.ac.uk/romeo/issn/0004-637X/ Author can archive publisher's version/PDF. Publisher's version/PDF may be used on any website or authors' institutional repository (Sherpa/Romeo as of 15/10/2018)
dc.publisherIOP Publishing
dc.relationhttp://purl.org/au-research/grants/arc/DP0559024
dc.relationhttp://purl.org/au-research/grants/arc/FF0561481
dc.rights© 2009. The American Astronomical Society.
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Astrometry; Binaries: close; Supernova remnants; Supernovae: general; Techniques: spectroscopic
dc.titleSubaru High-Resolution Spectroscopy of Star G in the Tycho Supernova Remnant
dc.typeJournal article
dcterms.accessRightsOpen Access
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage1672
local.bibliographicCitation.startpage1665
local.contributor.affiliationKerzendorf, Wolfgang, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationSchmidt, Brian, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationAsplund, Martin, Max Planck Institute for Astrophysics
local.contributor.affiliationNomoto, Ken'ichi, University of Tokyo
local.contributor.affiliationPodsiadlowski, Ph., Oxford University
local.contributor.affiliationFrebel, Anna, University of Texas
local.contributor.affiliationFesen, Robert A, Dartmouth College
local.contributor.affiliationYong, David, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.authoruidKerzendorf, Wolfgang, u4294536
local.contributor.authoruidSchmidt, Brian, u9500253
local.contributor.authoruidYong, David, u3207952
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3356449xPUB84
local.identifier.ariespublicationu4630950xPUB104
local.identifier.citationvolume701
local.identifier.doi10.1088/0004-637X/701/2/1665
local.identifier.essn1538-4357
local.identifier.scopusID2-s2.0-70549098333
local.identifier.thomsonID000268761500061
local.type.statusPublished Version

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