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dc.contributor.authorBonsor-Matthews, Amy
dc.contributor.authorFarihi, Jay
dc.contributor.authorWyatt, Mark
dc.contributor.authorvan Lieshout, Rik
dc.contributor.editorTremblay, P-E
dc.contributor.editorGänsicke, B
dc.contributor.editorMarsh, T
dc.date.accessioned2018-09-08T06:29:22Z
dc.date.available2018-09-08T06:29:22Z
dc.date.issued2017-03-31
dc.identifier.isbn978-1-58381-902-9
dc.identifier.issn1050-3390
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/279755
dc.description.abstractInfrared observations of polluted white dwarfs provide key insights into the accretion processes in action. The standard model for the observed infrared excesses is a flat, opaque, dust disc. The infrared observations are inconsistent with the presence of such a disc around all polluted white dwarfs. We discuss potential explanations for the absence of an infrared excess for many polluted white dwarfs.
dc.description.sponsorshipERC and Royal Society
dc.languageEnglish
dc.publisherSan Francisco Astronomical Society of the Pacific
dc.titleThe Dusty Accretion of Polluted White Dwarfs
dc.typeConference Object
prism.endingPage132
prism.publicationDate2017
prism.publicationName20TH EUROPEAN WHITE DWARF WORKSHOP
prism.startingPage127
prism.volume509
dc.identifier.doi10.17863/CAM.27125
dcterms.dateAccepted2016-09-01
rioxxterms.versionofrecord10.17863/CAM.27125
rioxxterms.licenseref.urihttp://www.rioxx.net/licenses/all-rights-reserved
rioxxterms.licenseref.startdate2017-03-31
dc.contributor.orcidBonsor-Matthews, Amy [0000-0002-8070-1901]
dc.contributor.orcidWyatt, Mark [0000-0001-9064-5598]
dc.publisher.urlhttp://adsabs.harvard.edu/abs/2017ASPC..509..127B
rioxxterms.typeConference Paper/Proceeding/Abstract
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2017ASPC..509..127B
pubs.conference-name20TH EUROPEAN WHITE DWARF WORKSHOP
pubs.conference-start-date2016-07-25
pubs.conference-finish-date2016-07-29
rioxxterms.freetoread.startdate2018-12-25


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