Effect of Dust Evaporation on the Fossil Magnetic Field of Young Stars and Their Accretion Disks

The theory of the fossil magnetic field of young stars and their accretion disks has been verified by comparing the observational data with the results of numerical simulations of the collapse of protostellar clouds. A new model of dust evaporation has been proposed, in which the parameter is not th...

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Veröffentlicht in:	Astronomy reports 2022-03, Vol.66 (3), p.200-220
Hauptverfasser:	Dudorov, A. E., Zamozdra, S. N.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Anisotropy Astronomy Cloud models Dust Dust effects Evaporation Evolution Grains Ionization Magnetic fields Mathematical models Numerical simulations Observations and Techniques Physics Physics and Astronomy Protostars Star formation Stellar magnetic fields
Online-Zugang:	Volltext
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