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The impact and evolution of magnetic confinement in hot stars

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no. 1
Z. Keszthelyi - G.a. Wade - V. Petit - G. Meynet - C. Georgy
Detaily:
Rok, strany: 2018, 124 - 128
Kľúčové slová:
stars: massive, stars: magnetic field
O článku:
Magnetic confinement of the winds of hot, massive stars has far-reaching consequences on timescales ranging from hours to Myr. Understanding the long-term effects of this interplay has already led to the identification of two new evolutionary pathways to form `heavy' stellar mass black holes and pair-instability supernova even at galactic metallicity. We are performing 1D stellar evolution model calculations that, for the first time, account for the surface effects and the time evolution of fossil magnetic fields. These models will be thoroughly confronted with observations and will potentially lead to a significant revision of the derived parameters of observed magnetic massive stars.
Ako citovať:
ISO 690:
Keszthelyi, Z., Wade, G., Petit, V., Meynet, G., Georgy, C. 2018. The impact and evolution of magnetic confinement in hot stars. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no.1, pp. 124-128. 1335-1842.

APA:
Keszthelyi, Z., Wade, G., Petit, V., Meynet, G., Georgy, C. (2018). The impact and evolution of magnetic confinement in hot stars. Contributions of the Astronomical Observatory Skalnaté Pleso, 48(1), 124-128. 1335-1842.