Protoplanetary Disks as (Possibly) Viscous Disks

Protoplanetary disks are believed to evolve on megayear timescales in a diffusive (viscous) manner as a result of angular momentum transport driven by internal stresses. Here we use a sample of 26 protoplanetary disks resolved by ALMA with measured (dust-based) masses and stellar accretion rates to...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	The Astrophysical journal Jg. 837; H. 2; S. 163 - 176
1. Verfasser:	Rafikov, Roman R.
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Philadelphia The American Astronomical Society 10.03.2017 IOP Publishing
Schlagworte:	ACCRETION DISKS accretion, accretion disks ANGULAR MOMENTUM Angular momentum transport Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Correlation COSMIC DUST Decoupling DENSITY DISTRIBUTION Field strength Fluid flow INSTABILITY IONIZATION LUMINOSITY MAGNETIC FIELDS MAGNETOHYDRODYNAMICS MASS Momentum transport Parameters Planet formation PLANETS planets and satellites: formation Protoplanetary disks PROTOPLANETS Residual stress RESIDUAL STRESSES SATELLITES Stellar winds Transport VISCOSITY
ISSN:	0004-637X, 1538-4357
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!