In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no. 1
Ch. Fendt
Detaily:
Rok, strany: 2018, 40 - 47
Kľúčové slová:
accretion, accretion disks, magnetohydrodynamics (MHD), ISM: jets and outflows, stars: mass loss, stars: pre-main sequence
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2018/Vol_48/No_1/pp40-47_abstract.html
O článku:
Recent results of magnetohydrodynamic (MHD) simulations are presented treating the launching of jets from young stellar object accretion disks. The simulations consider the evolution of magnetically diffusive disks that eject high-speed outflows. A few exemplary results are presented: (i) the disk structural evolution that leads to different launching conditions over time, (ii) a general interrelation between the disk magnetization at the outflow launching radius and the outflow asymptotic properties, (iii) jet launching within a self-generated disk magnetic field amplified by a disk mean field dynamo, and (iv) simulations of jets from orbiting jet sources.
Ako citovať:
ISO 690:
Fendt, C. 2018. Modeling the magnetized accretion and outflows in young stellar objects. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 48, no.1, pp. 40-47. 1335-1842.
APA:
Fendt, C. (2018). Modeling the magnetized accretion and outflows in young stellar objects. Contributions of the Astronomical Observatory Skalnaté Pleso, 48(1), 40-47. 1335-1842.