Magnetic Fields in Interacting Binaries

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no. 1

G. Briggs - L. Ferrario - C.a. Tout - D.t. Wickramasinghe

Detaily:

Rok, strany: 2018, 271 - 272

Kľúčové slová:

magnetic field, white dwarfs, binaries: general, novae, cataclysmic variables

URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2018/Vol_48/No_1/pp271-272_abstract.html

Full text

O článku:

Wickramasinghe et al. (2014) and Briggs et al. (2015) have proposed that the strong magnetic fields observed in some single white dwarfs (MWDs) are formed by an α—Ω dynamo driven by differential rotation when two stars, the more massive one with a degenerate core, merge during common envelope (CE) evolution (Ferrario et al., 2015b). We synthesise a population of binaries to investigate if fields in the magnetic cataclysmic variables (MCVs) may also originate during stellar interaction in the CE phase.

Ako citovať:

ISO 690:

Briggs, G., Ferrario, L., Tout, C., Wickramasinghe, D. 2018. Magnetic Fields in Interacting Binaries. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no.1, pp. 271-272. 1335-1842.

APA:

Briggs, G., Ferrario, L., Tout, C., Wickramasinghe, D. (2018). Magnetic Fields in Interacting Binaries. Contributions of the Astronomical Observatory Skalnaté Pleso, 48(1), 271-272. 1335-1842.