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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Bibliographic Details
Published in:	The Astrophysical journal Vol. 817; no. 1; pp. 35 - 52
Main Authors:	Lizano, S., Tapia, C., Boehler, Y., D'Alessio, P.
Format:	Journal Article
Language:	English
Published:	United Kingdom The American Astronomical Society 20.01.2016
Subjects:	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
Online Access:	Get full text
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