Vertical Shear Instability in the Solar Nebula

Min Kai Lin; Andrew N. Youdin

doi:10.1017/S174392131500589X

Vertical Shear Instability in the Solar Nebula

Min Kai Lin
, Andrew N. Youdin

Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

We quantify the thermodynamic requirement for the Vertical Shear Instability and evaluate its relevance to realistic protoplanetary disks as a potential route to hydrodynamic turbulence.

Original language	English (US)
Pages (from-to)	195-196
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	10
DOIs	https://doi.org/10.1017/S174392131500589X
State	Published - 2015

Keywords

accretion
accretion disks
hydrodynamics
instabilities
methods: analytical

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1017/S174392131500589X

Cite this

@article{ea989477eabe4ee2b96a24c31bd309dc,

title = "Vertical Shear Instability in the Solar Nebula",

abstract = "We quantify the thermodynamic requirement for the Vertical Shear Instability and evaluate its relevance to realistic protoplanetary disks as a potential route to hydrodynamic turbulence.",

keywords = "accretion, accretion disks, hydrodynamics, instabilities, methods: analytical",

author = "Lin, \{Min Kai\} and Youdin, \{Andrew N.\}",

note = "Publisher Copyright: {\textcopyright} 2016 International Astronomical Union.",

year = "2015",

doi = "10.1017/S174392131500589X",

language = "English (US)",

volume = "10",

pages = "195--196",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

}

TY - JOUR

T1 - Vertical Shear Instability in the Solar Nebula

AU - Lin, Min Kai

AU - Youdin, Andrew N.

PY - 2015

Y1 - 2015

N2 - We quantify the thermodynamic requirement for the Vertical Shear Instability and evaluate its relevance to realistic protoplanetary disks as a potential route to hydrodynamic turbulence.

AB - We quantify the thermodynamic requirement for the Vertical Shear Instability and evaluate its relevance to realistic protoplanetary disks as a potential route to hydrodynamic turbulence.

KW - accretion

KW - accretion disks

KW - hydrodynamics

KW - instabilities

KW - methods: analytical

UR - https://www.scopus.com/pages/publications/84956471140

UR - https://www.scopus.com/pages/publications/84956471140#tab=citedBy

U2 - 10.1017/S174392131500589X

DO - 10.1017/S174392131500589X

M3 - Article

AN - SCOPUS:84956471140

SN - 1743-9213

VL - 10

SP - 195

EP - 196

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

ER -

Vertical Shear Instability in the Solar Nebula

Abstract

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this