PopCORN: Hunting down the differences between binary population synthesis codes

dc.contributor.authorToonen, S.
dc.contributor.authorClaeys, J. S. W.
dc.contributor.authorMennekens, N.
dc.contributor.authorRuiter, Ashley
dc.date.accessioned2018-11-29T22:52:08Z
dc.date.available2018-11-29T22:52:08Z
dc.date.issued2014
dc.date.updated2018-11-29T07:43:54Z
dc.description.abstractBinary population synthesis (BPS) modelling is a very effective tool to study the evolution and properties of various types of close binary systems. The uncertainty in the parameters of the model and their effect on a population can be tested in a statistical way, which then leads to a deeper understanding of the underlying (sometimes poorly understood) physical processes involved. Several BPS codes exist that have been developed with different philosophies and aims. Although BPS has been very successful for studies of many populations of binary stars, in the particular case of the study of the progenitors of supernovae Type Ia, the predicted rates and ZAMS progenitors vary substantially between different BPS codes.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/152089
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.titlePopCORN: Hunting down the differences between binary population synthesis codes
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issueA14
local.contributor.affiliationToonen, S., Radboud University
local.contributor.affiliationClaeys, J. S. W., Radboud University
local.contributor.affiliationMennekens, N., Vrije Universiteit Brussel
local.contributor.affiliationRuiter, Ashley, College of Science, ANU
local.contributor.authoruidRuiter, Ashley, u4147637
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationu4571891xPUB22
local.identifier.citationvolume562
local.identifier.doi10.1051/0004-6361/201321576
local.identifier.scopusID2-s2.0-84893264192
local.identifier.thomsonID000332161800023
local.type.statusPublished Version

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