In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no. 1
H. Korhonen
Details:
Year, pages: 2018, 180 - 186
Keywords:
stars: atmospheres, stars: evolution, stars: late-type, stars: magnetic field
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2018/Vol_48/No_1/pp180-186_abstract.html
About article:
The recent years have brought great advances in our knowledge of magnetic fields in cool giant and supergiant stars. For example, starspots have been directly imaged on the surface of an active giant star using optical interferometry, and magnetic fields have been detected in numerous slowly rotating giants and even on supergiants. Here, I review what is currently known of the magnetism in cool giant and supergiant stars, and discuss the origin of these fields and what is theoretically known about them.
How to cite:
ISO 690:
Korhonen, H. 2018. Magnetic fields of cool giant and supergiant stars: models versus observations. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no.1, pp. 180-186. 1335-1842.
APA:
Korhonen, H. (2018). Magnetic fields of cool giant and supergiant stars: models versus observations. Contributions of the Astronomical Observatory Skalnaté Pleso, 48(1), 180-186. 1335-1842.