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Tracking down R Coronae Borealis stars from their mid-infrared WISE colours

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dc.contributor.authorTisserand, Patrick
dc.date.accessioned2015-12-10T23:25:16Z
dc.date.issued2012
dc.date.updated2016-02-24T08:47:10Z
dc.description.abstractContext. R Coronae Borealis stars (RCBs) are hydrogen-deficient and carbon-rich supergiant stars. They are very rare, with only ∼50 actually known in our Galaxy. Interestingly, RCBs are strongly suspected of being the evolved merger product of two white
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/67560
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectCatalogs
dc.subjectCircumstellar matter
dc.subjectInfrared: stars
dc.subjectStars: AGB and post-AGB
dc.subjectStars: carbon
dc.subjectAmorphous carbon
dc.subjectColor
dc.subjectGalaxies
dc.subjectHydrogen
dc.subjectInfrared devices
dc.subjectStars Catalogs
dc.subjectCircumstellar matter
dc.subjectInfrared: stars
dc.subjectStars: AGB and post-AGB
dc.subjectStars: carbon
dc.titleTracking down R Coronae Borealis stars from their mid-infrared WISE colours
dc.typeJournal article
local.contributor.affiliationTisserand, Patrick, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidTisserand, Patrick, u4336119
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB1477
local.identifier.citationvolume539
local.identifier.doi10.1051/0004-6361/201117874
local.identifier.scopusID2-s2.0-84857406576
local.identifier.thomsonID000303262000058
local.type.statusPublished Version

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