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dc.contributor.editorCastanheira, B.
dc.contributor.editorVanderbosch, Z.
dc.contributor.editorMontgomery, M.
dc.creatorBédard, A.
dc.creatorBergeron, P.
dc.creatorFontaine, G.
dc.date.accessioned2018-12-17T15:06:54Z
dc.date.available2018-12-17T15:06:54Z
dc.date.issued2018-07
dc.identifierdoi:10.15781/T2TX35S7Q
dc.identifier.urihttp://hdl.handle.net/2152/71581
dc.descriptionThe 21st European Workshop on White Dwarfs was held in Austin, TX from July 23rd to 27th of 2018en_US
dc.description.abstractWe present updated atmospheric parameters for all DA, DB, and DO white dwarfs in the complete sample of the Palomar-Green survey. In particular, we perform a spectroscopic analysis of the DO stars using our new set of non-LTE model atmosphere calculations. We then compute an improved luminosity function of the Palomar-Green sample, including the DO stars for the first time, which allows us to study the variations in the numbers of hydrogen- and helium-atmosphere white dwarfs along a large part of the cooling sequence. We demonstrate that the so-called float-up model successfully explains the spectral evolution of the majority of white dwarfs.en_US
dc.language.isoengen_US
dc.relation.ispartof21st European White Dwarf Workshopen_US
dc.subjectwhite dwarfsen_US
dc.subjectPalomar-Green surveyen_US
dc.subjectluminosity functionen_US
dc.titleRevisiting the White Dwarf Luminosity Function from the Palomar-Green Surveyen_US
dc.typeConference paperen_US
dc.description.departmentAstronomyen_US
dc.rights.restrictionOpenen_US


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