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dc.contributor.editorCastanheira, B.
dc.contributor.editorVanderbosch, Z.
dc.contributor.editorMontgomery, M.
dc.creatorIsern, J.
dc.creatorBravo, E.
dc.date.accessioned2018-12-19T16:37:03Z
dc.date.available2018-12-19T16:37:03Z
dc.date.issued2018-07
dc.identifierdoi:10.15781/T2902024F
dc.identifier.urihttp://hdl.handle.net/2152/71593
dc.descriptionThe 21st European Workshop on White Dwarfs was held in Austin, TX from July 23rd to 27th of 2018en_US
dc.description.abstractThe analysis of noble gases in primitive meteorites has shown the existence of anomalous isotopic abundances when compared with the average Solar System values. In particular it has been found that some graphite grains contain an unexpected high abundance of neon-22. This excess of neon- 22 is usually attributed to the radioactive decay of sodium-22 produced in the O/Ne burning layer of a core collapse supernova. In this talk we speculate about a different origin, the disruption of a crystallized white dwarf by a compact object (white dwarf, neutron star, or black hole).en_US
dc.language.isoengen_US
dc.relation.ispartof21st European White Dwarf Workshopen_US
dc.subjectwhite dwarfsen_US
dc.subjectneon-22en_US
dc.subjectwhite dwarf collisionen_US
dc.titleWhite dwarf collisions and the meteoritic Ne-E anomalyen_US
dc.typeConference paperen_US
dc.description.departmentAstronomyen_US
dc.rights.restrictionOpenen_US


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