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dc.contributor.editorCastanheira, B.
dc.contributor.editorVanderbosch, Z.
dc.contributor.editorMontgomery, M.
dc.creatorNeunteufel, P.
dc.creatorYoon, S.C.
dc.creatorLanger, N.
dc.date.accessioned2018-12-19T16:43:33Z
dc.date.available2018-12-19T16:43:33Z
dc.date.issued2018-07
dc.identifierdoi:10.15781/T21J97V0D
dc.identifier.urihttp://hdl.handle.net/2152/71595
dc.descriptionThe 21st European Workshop on White Dwarfs was held in Austin, TX from July 23rd to 27th of 2018en_US
dc.description.abstractBinary systems composed of one helium-rich nondegenerate star and one carbon-oxygen white dwarf (He+CO) have long been considered a promising progenitor candidate for a number of astrophysical transients like archetypical supernovae of the type Ia, Iax, and a number of less luminous phenomena, such as He-novae and AM CVn stars. Among the proposed mechanisms capable of initiating a detonation of the degenerate core of the WD, the sub-Chandrasekhar mass double detonation has received increased attention in recent years. We present the results of a number of numerical simulations on the evolution of helium accreting CO WDs with an emphasis on the effects of differential rotation and magnetic fields in the context of the Spruit-Tayler (ST) dynamo. We present findings of two papers: Neunteufel et al. (2017) and (forthcoming) Neunteufel et al. (2018)en_US
dc.language.isoengen_US
dc.relation.ispartof21st European White Dwarf Workshopen_US
dc.subjectwhite dwarfsen_US
dc.subjectdouble detonationsen_US
dc.subjecthelium accreting CO WDsen_US
dc.titleMagnetic Torques Imply Fewer Double Detonationsen_US
dc.typeConference paperen_US
dc.description.departmentAstronomyen_US
dc.rights.restrictionOpenen_US


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