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Observational properties of magnetic white dwarfs

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dc.contributor.authorFerrario, Lilia
dc.contributor.editorRuffini, R.
dc.contributor.editorBianchi, M.
dc.contributor.editorJantzen, R. T.
dc.coverage.spatialRome, Italy
dc.date.accessioned2022-11-28T01:26:40Z
dc.date.available2022-11-28T01:26:40Z
dc.date.createdJuly 12-18 2015
dc.date.issued2018
dc.date.updated2021-11-28T07:29:39Z
dc.description.abstractThere are no known examples of magnetic white dwarfs with fields larger than ∼ 3 MG paired with a non-degenerate companion in detached binary systems. The suggestion is that highly magnetic, isolated white dwarfs may originate from stars that coalesce during common envelope evolution while those stars that emerge from a common envelope on a close orbit may evolve into double degenerate systems consisting of two white dwarfs, one or both magnetic. The presence of planets or planetary debris around white dwarfs is also a new and exciting area of research that may give us important clues on the formation of first and second generation planetary systems, since these place unique signatures in the spectra of white dwarfs.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.isbn978-981322659-3en_AU
dc.identifier.urihttp://hdl.handle.net/1885/280447
dc.language.isoen_AUen_AU
dc.provenanceThis is an Open Access proceedings volume published by World Scientific Publishing Company. It is distributed under the terms of the Creative Commons Attribution 4.0 (CC-BY) License.en_AU
dc.publisherWorld Scientific Publishing Co Pte Ltden_AU
dc.relation.ispartofseries14th Marcel Grossman Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theoriesen_AU
dc.rights© The Editorsen_AU
dc.rights.licenseCreative Commons Attribution 4.0 International Licenseen_AU
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_AU
dc.source14th Marcel Grossman Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories, Proceedingsen_AU
dc.subjectWhite dwarfsen_AU
dc.subjectmagnetic fieldsen_AU
dc.subjectdouble degeneratesen_AU
dc.subjectplanetsen_AU
dc.titleObservational properties of magnetic white dwarfsen_AU
dc.typeConference paperen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.lastpage4280en_AU
local.bibliographicCitation.startpage4271en_AU
local.contributor.affiliationFerrario, Lilia, College of Science, ANUen_AU
local.contributor.authoruidFerrario, Lilia, u8513121en_AU
local.description.notesImported from ARIESen_AU
local.description.refereedYes
local.identifier.absfor510109 - Stellar astronomy and planetary systemsen_AU
local.identifier.absfor490399 - Numerical and computational mathematics not elsewhere classifieden_AU
local.identifier.absseo280120 - Expanding knowledge in the physical sciencesen_AU
local.identifier.absseo280118 - Expanding knowledge in the mathematical sciencesen_AU
local.identifier.ariespublicationu3102795xPUB1732en_AU
local.identifier.doi10.1142/9789813226609_0572en_AU
local.identifier.scopusID2-s2.0-85059063722
local.publisher.urlhttps://www.worldscientific.com/en_AU
local.type.statusPublished Versionen_AU

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