Statistics of magnetic fields on OBA stars

dc.contributor.authorKholtygin, A. F.
dc.contributor.authorHubrig, S.
dc.contributor.authorDrake, N. A.
dc.contributor.authorSudnik, N. P.
dc.contributor.authorDushin, V. V.
dc.date.accessioned2016-12-11T12:40:20Z
dc.date.available2016-12-11T12:40:20Z
dc.date.issued2014
dc.description.abstractStarting from recent measurements, we studied the statistical properties of the magnetic fields of OBA stars. As one of the statistically significant characteristics of the magnetic field we use the average effective magnetic field of the star, ⟨B⟩. We then investigated the distribution function f (⟨B⟩) of the magnetic fields of OBA stars. This function has a power-law dependence on ⟨B⟩, with an index of 2–3 and a fast decrease for ⟨B⟩ ≤ 300G for B–A stars and ⟨B⟩ ≤ 80G for O stars.ru_RU
dc.identifier.urihttp://elib.bspu.by/handle/doc/17611
dc.language.isoenru_RU
dc.relation.ispartofseriesProc. of conf. «Putting A Stars into Context: Evolution, Environment, and Related Stars», Moscow, Russia, June 2013;p. 403
dc.subjectБГПУru_RU
dc.subjectOBA starsru_RU
dc.subjectstatistical propertiesru_RU
dc.subjectmagnetic fieldsru_RU
dc.titleStatistics of magnetic fields on OBA starsru_RU
dc.typeArticleru_RU

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