In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 50, no. 2
E. Paunzen
Details:
Year, pages: 2020, 570 - 573
Language: eng
Keywords:
binaries: general, stars: chemically peculiar, stars: magnetic fields
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2020/Vol_50/No_2/pp570-573_abstract.html
About article:
Magnetic chemically peculiar stars of the upper main sequence are slowly rotating early B to early F-type objects with elemental overabundances of several orders of magnitude compared to the Sun. The driving mechanism is diffusion in the calm stellar atmosphere intensified by the presence of a stable organized magnetic field. The binary fraction is vital to understanding the formation and evolution of these objects as well as possible operating angular momentum loss mechanisms. The available literature on the binary fraction is reviewed and a list of needed future working steps is presented.
How to cite:
ISO 690:
Paunzen, E. 2020. Binary fraction of magnetic chemically peculiar stars. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 50, no.2, pp. 570-573. 1335-1842. DOI: https://doi.org/10.31577/caosp.2020.50.2.570
APA:
Paunzen, E. (2020). Binary fraction of magnetic chemically peculiar stars. Contributions of the Astronomical Observatory Skalnaté Pleso, 50(2), 570-573. 1335-1842. DOI: https://doi.org/10.31577/caosp.2020.50.2.570
About edition:
Publisher: Astronomical Institute, Slovak Academy of Sciences
Published: 1. 3. 2020
Rights:
