The local stability of accretion disk models with considering the role of various viscosity and cooling mechanisms

ISSN： 0004-640X

Source： Astrophysics and Space Science, Vol.348, Iss.1, 2013-11, pp. : 143-153

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

Stability of Accretion Models

By Pustil'nik L.A.

Astrophysics and Space Science, Vol. 252, Iss. 1-2, 1997-01 ,pp. : 353-362

Springer Publishing Company

Access to resources Recommend Favorite

The role of toroidal magnetic field in the stability of accretion disks with alpha viscosity and other viscosities

By Khosravi A. Khesali A.

Astrophysics and Space Science, Vol. 350, Iss. 2, 2014-04 ,pp. : 645-655

Springer Publishing Company

Access to resources Recommend Favorite

Structure and stability of magnetized accretion disks with anomalous viscosity

By Zhou Ai-ping Liu Han-fa Gao Jin-xia

Astrophysics and Space Science, Vol. 348, Iss. 2, 2013-12 ,pp. : 337-343

Springer Publishing Company

Access to resources Recommend Favorite

Structure and stability of a thin protostar disk with anomalous viscosity

By Lin Fu-Jun

Astrophysics and Space Science, Vol. 335, Iss. 2, 2011-10 ,pp. : 469-474

Springer Publishing Company

Access to resources Recommend Favorite

Formation of the accretion disk in the SS 433 system with explicit radiative cooling, convective heat conduction, and radiation pressure

By Nazarenko V. Glazunova L.

Astronomy Reports, Vol. 49, Iss. 10, 2005-10 ,pp. : 826-836

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite