A simple and accurate approximation for the Q stability parameter in multicomponent and realistically thick discs

Author： Romeo Alessandro B. Falstad Niklas

ISSN： 0035-8711

Source： Monthly Notices of the Royal Astronomical Society, Vol.433, Iss.2, 2013-01, pp. : 1389-1397

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

The effective stability parameter for two-component galactic discs: is

By Romeo Alessandro B. Wiegert Joachim

Monthly Notices of the Royal Astronomical Society, Vol. 416, Iss. 2, 2011-09 ,pp. : 1191-1196

Oxford University Press

Access to resources Recommend Favorite

Radial migration in galactic thick discs

By Solway Michael Sellwood J. A. Schönrich Ralph

Monthly Notices of the Royal Astronomical Society, Vol. 422, Iss. 2, 2012-05 ,pp. : 1363-1383

Oxford University Press

Access to resources Recommend Favorite

Type I migration in optically thick accretion discs

By Yamada K. Inaba S.

Monthly Notices of the Royal Astronomical Society, Vol. 424, Iss. 4, 2012-08 ,pp. : 2746-2756

Oxford University Press

Access to resources Recommend Favorite

Jet launching from accretion discs in the local approximation

By Ogilvie Gordon I.

Monthly Notices of the Royal Astronomical Society, Vol. 423, Iss. 2, 2012-06 ,pp. : 1318-1324

Oxford University Press

Access to resources Recommend Favorite

Virial sequences for thick discs and haloes: flattening and global anisotropy

By Agnello A. Evans N. W.

Monthly Notices of the Royal Astronomical Society, Vol. 422, Iss. 2, 2012-05 ,pp. : 1767-1778

Oxford University Press

Access to resources Recommend Favorite