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dc.contributor.authorVennes, S.
dc.contributor.authorKawka, Adela
dc.contributor.authorFerrario, L.
dc.contributor.authorPaunzen, E.
dc.date.accessioned2019-02-19T04:14:10Z
dc.date.available2019-02-19T04:14:10Z
dc.date.created2019-02-19T03:58:18Z
dc.date.issued2018
dc.identifier.citationVennes, S. and Kawka, A. and Ferrario, L. and Paunzen, E. 2018. Observing and modelling magnetic fields in white dwarfs. Contributions of the Astronomical Observatory Skalnate Pleso. 48 (1): pp. 307-311.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/73554
dc.description.abstract

Our ongoing spectroscopic survey of high proper motion stars is a rich source of new magnetic white dwarfs. We present a few examples among cool white dwarfs showing the effect of field strength and geometry on the observed optical spectrum. Modelling of hydrogen and heavy element spectral lines reveals a range of uniform or markedly offset dipole fields in these objects.

dc.titleObserving and modelling magnetic fields in white dwarfs
dc.typeJournal Article
dcterms.source.volume48
dcterms.source.number1
dcterms.source.startPage307
dcterms.source.endPage311
dcterms.source.issn1335-1842
dcterms.source.titleContributions of the Astronomical Observatory Skalnate Pleso
curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusFulltext not available


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