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WD1953-011: a magnetic white dwarf with peculiar field structure

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dc.contributor.authorMaxted, P F L
dc.contributor.authorFerrario, Lilia
dc.contributor.authorMarsh, T R
dc.contributor.authorWickramasinghe, Dayal
dc.date.accessioned2015-12-13T23:18:00Z
dc.date.available2015-12-13T23:18:00Z
dc.date.issued2000
dc.date.updated2015-12-12T08:55:08Z
dc.description.abstractWe present Hα spectra of the magnetic white dwarf star WD 1953-011 which confirm the presence of the broad Zeeman components corresponding to a field strength of ∼500 kG found by Maxted & Marsh. We also find that the line profile is variable over a tim
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/89966
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Stars: individual: WD 1953-011; Stars: magnetic fields; White dwarfs
dc.titleWD1953-011: a magnetic white dwarf with peculiar field structure
dc.typeJournal article
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpageL44
local.bibliographicCitation.startpageL41
local.contributor.affiliationMaxted, P F L, University of Southampton
local.contributor.affiliationFerrario, Lilia, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMarsh, T R, University of Southampton
local.contributor.affiliationWickramasinghe, Dayal, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidFerrario, Lilia, u8513121
local.contributor.authoruidWickramasinghe, Dayal, u7600909
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub20216
local.identifier.citationvolume315
local.identifier.scopusID2-s2.0-0039683615
local.type.statusPublished Version

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