In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
E. Gerth - Yu.v. Glagolevskij
Details:
Year, pages: 2008, 407 - 408
Keywords:
stars: magnetic fields, methods: analytical, stars: individual: ν Cep
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_2/pp407-408_abstract.html
About article:
The magnetically sensitive atmosphere of a star is an ideal detector
of the magnetic field penetrating the atmospheric layer -
regardless of whether the field source is inside or outside the star. Most magnetic stars possess their own
magnetic field sources in their interiors, and one usually neglects the possibility of
externally caused influences of magnetic fields. Only powerful interior or nearby
magnetic sources may influence detectably the atmosphere
of a star with a sufficiently large surface. An externally
influenced magnetic field can be found in a binary system consisting
of a non-magnetic giant with a magnetic dwarf
companion.
How to cite:
ISO 690:
Gerth, E., Glagolevskij, Y. 2008. The magnetic field generated by sources inside and outside the star. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 407-408. 1335-1842.
APA:
Gerth, E., Glagolevskij, Y. (2008). The magnetic field generated by sources inside and outside the star. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 407-408. 1335-1842.