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dc.contributor.authorCasewell, Sarah L.
dc.contributor.authorBurleigh, Matt R.
dc.contributor.authorDobbie, Paul D.
dc.contributor.authorNapiwotzki, Ralf
dc.contributor.editorSchuh, S
dc.contributor.editorDrechsel, H
dc.contributor.editorHeber, U
dc.date.accessioned2011-11-22T13:01:08Z
dc.date.available2011-11-22T13:01:08Z
dc.date.issued2011
dc.identifier.citationCasewell , S L , Burleigh , M R , Dobbie , P D & Napiwotzki , R 2011 , Evolved solar systems in Praesepe . in S Schuh , H Drechsel & U Heber (eds) , Planetary Systems Beyond the Main Sequence . vol. 1331 , AIP Conference Proceedings , American Institute of Physics , Melville , pp. 292-296 . https://doi.org/10.1063/1.3556214
dc.identifier.isbn978-0-7354-0886-9
dc.identifier.otherPURE: 457655
dc.identifier.otherPURE UUID: bebb72a0-7c78-4218-b99e-bb978daa0332
dc.identifier.otherWOS: 000290243400034
dc.identifier.otherScopus: 79953864241
dc.identifier.urihttp://hdl.handle.net/2299/7085
dc.description"Copyright 2011 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics." Original paper can be found at: http://scitation.aip.org/"
dc.description.abstractWe have obtained near-IR photometry for the 11 Praesepe white dwarfs, to search for an excess indicative of a dusty debris disk. All the white dwarfs are in the DAZ temperature regime, however we find no indications of a disk around any white dwarf. We have, however determined that the radial velocity variable white dwarf WD0837+185 could have an unresolved T8 dwarf companion that would not be seen as a near-IR excess.en
dc.format.extent5
dc.language.isoeng
dc.publisherAmerican Institute of Physics
dc.relation.ispartofPlanetary Systems Beyond the Main Sequence
dc.relation.ispartofseriesAIP Conference Proceedings
dc.rightsOpen
dc.subjectWhite Dwarfs
dc.subjectclusters
dc.titleEvolved solar systems in Praesepeen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2011
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1063/1.3556214
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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