On the Observation Data which Confirm Binary Nature of Magnetic Chemically Peculiar Stars
Abstract
A new evolutionary scenario of the roAp Przybylski star (HD101065) that revolves with a neutron star (pulsar) in the plane which is perpendicular to the line of sight that we proposed earlier can be extended to other magnetic stars, too. Observations in radio, X-ray, and IR regions, properties of the magnetic chemically peculiar stars, as well as phenomenon of roAp stars, can be explained within the proposed hypothesis.
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Гопка В.Ф О наблюдательных фактах, подтверждающих двойственность магнитных химически пекулярных звезд / В.Ф. Гопка, О.М. Ульянов, С.M. Андриевский // Радиофизика и радиоастрономия. — 2008. — Т. 13, № 3. Специальный выпуск. — С. 43-57.
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