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Constraints on the pairing properties of main-sequence stars from observations of white dwarfs in binary systems

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dc.contributor.authorFerrario, Lilia
dc.date.accessioned2015-12-13T22:22:28Z
dc.date.issued2012
dc.date.updated2016-02-24T09:06:22Z
dc.description.abstractObservations of main-sequence stars conducted over the last several decades have clearly shown that something like 50 per cent of stars of spectral types G and F occur in multiple systems. For earlier spectral types, the incidence of multiplicity is even
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/72269
dc.publisherBlackwell Publishing Ltd
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Binaries: general; Stars: formation; Stars: low-mass; White dwarfs
dc.titleConstraints on the pairing properties of main-sequence stars from observations of white dwarfs in binary systems
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage2506
local.bibliographicCitation.startpage2500
local.contributor.affiliationFerrario, Lilia, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidFerrario, Lilia, u8513121
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absseo970101 - Expanding Knowledge in the Mathematical Sciences
local.identifier.ariespublicationf5625xPUB3159
local.identifier.citationvolume426
local.identifier.doi10.1111/j.1365-2966.2012.21836.x
local.identifier.scopusID2-s2.0-84881114216
local.identifier.thomsonID000310063900060
local.type.statusPublished Version

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