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A high-resolution spectroscopic search for the remaining donor for Tycho'S supernova

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dc.contributor.authorKerzendorf, Wolfgang
dc.contributor.authorYong, David
dc.contributor.authorSimon, J
dc.contributor.authorJeffery, Simon C
dc.contributor.authorAnderson, Jay
dc.contributor.authorPodsiadlowski, Ph.
dc.contributor.authorGal-Yam, Avishay
dc.contributor.authorSilverman, J. M.
dc.contributor.authorFilippenko, Alexei
dc.contributor.authorNomoto, Ken'ichi
dc.contributor.authorMurphy, Simon
dc.contributor.authorBessell, Michael
dc.contributor.authorVenn, Kim
dc.contributor.authorFoley, Ryan
dc.date.accessioned2015-12-13T22:27:12Z
dc.date.issued2013
dc.date.updated2016-02-24T09:18:11Z
dc.description.abstractIn this paper, we report on our analysis using Hubble Space Telescope astrometry and Keck-I HIRES spectroscopy of the central six stars of Tycho's supernova remnant (SN 1572). With these data, we measured the proper motions, radial velocities, rotational
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/73837
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: ISM: supernova remnants; supernovae: individual (SN1572)
dc.titleA high-resolution spectroscopic search for the remaining donor for Tycho'S supernova
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.startpage19
local.contributor.affiliationKerzendorf, Wolfgang, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationYong, David, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSchmidt, Brian, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSimon, J, Observatories of the Carnegie Institution of Washington
local.contributor.affiliationJeffery, Simon C, Armagh Observatory
local.contributor.affiliationAnderson, Jay, Space Telescope Science Institute
local.contributor.affiliationPodsiadlowski, Ph., Oxford University
local.contributor.affiliationGal-Yam, Avishay, Weizmann Institute of Science
local.contributor.affiliationSilverman, J. M., University of California
local.contributor.affiliationFilippenko, Alexei, University of California
local.contributor.affiliationNomoto, Ken'ichi, University of Tokyo
local.contributor.affiliationMurphy, Simon, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationVenn, Kim, University of Victoria
local.contributor.affiliationFoley, Ryan, University of California
local.contributor.authoruidKerzendorf, Wolfgang, u4294536
local.contributor.authoruidYong, David, u3207952
local.contributor.authoruidSchmidt, Brian, u9500253
local.contributor.authoruidMurphy, Simon, u4203307
local.contributor.authoruidBessell, Michael, u6900904
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB3853
local.identifier.citationvolume774
local.identifier.doi10.1088/0004-637X/774/2/99
local.identifier.scopusID2-s2.0-84883625505
local.identifier.thomsonID000323888900008
local.type.statusPublished Version

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