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dc.contributor.editorCastanheira, B.
dc.contributor.editorVanderbosch, Z.
dc.contributor.editorMontgomery, M.
dc.creatorSzkody, Paula
dc.creatorMukadam, Anjum
dc.date.accessioned2018-12-19T16:48:03Z
dc.date.available2018-12-19T16:48:03Z
dc.date.issued2018-07
dc.identifierdoi:10.15781/T2S17TD0H
dc.identifier.urihttp://hdl.handle.net/2152/71597
dc.descriptionThe 21st European Workshop on White Dwarfs was held in Austin, TX from July 23rd to 27th of 2018en_US
dc.description.abstractSince the last white dwarf workshop, there is continuing evidence that long (hrs to days) periodicities are being found in white dwarfs that are undergoing accretion in close binary systems. Pulsation modes remain a possible explanation but proof remains elusive. We will compare the known properties of accreting, pulsating white dwarfs with those in ZZ Ceti stars. While sky surveys continue to proliferate, the discovery of accreting pulsators is not rising proportionally. Reasons for this discrepancy as well as future needs are discussed.en_US
dc.language.isoengen_US
dc.relation.ispartof21st European White Dwarf Workshopen_US
dc.subjectwhite dwarfsen_US
dc.subjectaccreting white dwarfsen_US
dc.subjectpulsationen_US
dc.titleAn Update on Pulsations in Accreting White Dwarfsen_US
dc.typeConference paperen_US
dc.description.departmentAstronomyen_US
dc.rights.restrictionOpenen_US


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