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New Magellanic Cloud R Coronae Borealis and DY Persei type stars from the EROS-2 database: The connection between RCBs, DYPers, and ordinary carbon stars

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dc.contributor.authorTisserand, Patrick
dc.contributor.authorWood, Peter R.
dc.contributor.authorMarquette, J. B.
dc.contributor.authorAfonso, C.
dc.contributor.authorAlbert, J. N.
dc.contributor.authorAnderson, J.
dc.contributor.authorAnsari, R.
dc.contributor.authorAubourg, E.
dc.contributor.authorBareyre, P.
dc.contributor.authorBeaulieu, J.-P.
dc.contributor.authorCharlot, X.
dc.contributor.authorCoutures, C.
dc.contributor.authorFerlet, R.
dc.date.accessioned2015-12-08T22:19:56Z
dc.date.issued2009
dc.date.updated2016-02-24T09:55:25Z
dc.description.abstractContext. R Coronae Borealis stars (RCB) are a rare type of evolved carbon-rich supergiant stars that are increasingly thought to result from the merger of two white dwarfs, called the Double degenerate scenario. This scenario is also studied as a source,
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/31776
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Absolute luminosity; Abundance analysis; Borealis; Broad bands; Carbon rich; Carbon stars; Circumstellar; Colour-magnitude diagrams; Light curves; Magellanic Clouds; Midinfrared; Optical spectroscopy; Post-AGB; Shell temperatures; Spectral energy distribu Magellanic Clouds; Stars: AGB and post-AGB; Stars: carbon; Supergiants
dc.titleNew Magellanic Cloud R Coronae Borealis and DY Persei type stars from the EROS-2 database: The connection between RCBs, DYPers, and ordinary carbon stars
dc.typeJournal article
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage998
local.bibliographicCitation.startpage985
local.contributor.affiliationTisserand, Patrick, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMarquette, J B, Universite Pierre & Marie Curie
local.contributor.affiliationAfonso, C, Centre d Etudes de Saclay
local.contributor.affiliationAlbert, J.N., Universite de Paris-Sud
local.contributor.affiliationAnderson, J, Copenhagen University
local.contributor.affiliationAnsari, R, CNRS Universite Paris-Sud
local.contributor.affiliationAubourg, E, CEA-Saclay
local.contributor.affiliationBareyre, P, CEA-Saclay
local.contributor.affiliationBeaulieu, J.-P, Universite Pierre et Marie Curie (CRNS)
local.contributor.affiliationCharlot, X, CEA-Saclay
local.contributor.affiliationCoutures, C, CEA-Saclay
local.contributor.affiliationFerlet, R, Universite Pierre & Marie Curie
local.contributor.authoruidTisserand, Patrick, u4336119
local.contributor.authoruidWood, Peter R, u7900259
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3356449xPUB86
local.identifier.citationvolume501
local.identifier.doi10.1051/0004-6361/200911808
local.identifier.scopusID2-s2.0-76349084195
local.identifier.thomsonID000268292200015
local.type.statusPublished Version

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