VERTICAL STRUCTURE OF MAGNETIZED ACCRETION DISKS AROUND YOUNG STARS

ABSTRACT We model the vertical structure of the magnetized accretion disks that are subject to viscous and resistive heating and irradiation by the central star. We apply our formalism to the radial structure of the magnetized accretion disks that are threaded by the poloidal magnetic field dragged...

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Vydané v:	The Astrophysical journal Ročník 817; číslo 1; s. 35 - 52
Hlavní autori:	Lizano, S., Tapia, C., Boehler, Y., D'Alessio, P.
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	United Kingdom The American Astronomical Society 20.01.2016
Predmet:	ACCRETION DISKS accretion, accretion disks ASPECT RATIO ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Balances (scales) COMPARATIVE EVALUATIONS Disks EMISSION Formalism Heating Irradiation ISM: magnetic fields MAGNETIC FIELDS MAGNETIZATION MAGNETOHYDRODYNAMICS magnetohydrodynamics (MHD) MASS protoplanetary disks PROTOPLANETS PROTOSTARS ROTATION STAR EVOLUTION STARS stars: formation STELLAR ATMOSPHERES VELOCITY
ISSN:	0004-637X, 1538-4357
On-line prístup:	Získať plný text
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