On the viscosity in accretion disks

Details On the viscosity in accretion disks On the viscosity in accretion disks

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..393d&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 393-396 (SEE N90-25711 19-89)

Physics

Accretion Disks, Convection, Stellar Mass Accretion, Stellar Models, Viscosity, Dwarf Novae, Star Formation, Stellar Interiors, Stellar Physics, Structures

Scientific paper

The physical processes that cause the viscosity in accretion disks are considered. A newly proposed approach that couples viscosity and convection are discussed. It is assumed that only one turbulent process underlies both processes and that it manifests itself in two different geometrical directions in physically quite distinct processes. The models calculated using this ansatz are capable of describing the unstable disk structure without introducing an ad-hoc viscosity parameter, in convective regions, and explaining the UV delay that is observed in some dwarf novae.

Affiliated with

Also associated with

No associations

Rating

On the viscosity in accretion disks does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with On the viscosity in accretion disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the viscosity in accretion disks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1614622