Comparison Between Two- and Three-dimensional Modeling of the Structure of an Accretion Disk in a Binary System

Details Comparison Between Two- and Three-dimensional Modeling of the Structure of an Accretion Disk in a Binary System Comparison Between Two- and Three-dimensional Modeling of the Structure of an Accretion Disk in a Binary System

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003arep...47...11a&link_type=abstract

Astronomy Reports, vol. 47, Issue 1, p.11-19

Astronomy and Astrophysics

Astronomy

Scientific paper

We compare two-and three-dimensional modeling of gas-dynamical processes
in the accretion disk of a binary system. The origin of spiral waves and
the loss of the angular momentum related to them are considered. It is
concluded that a steady state of the disk cannot exist without taking
into account t he gas inflow from the donor star.

Affiliated with

Also associated with

No associations

Rating

Comparison Between Two- and Three-dimensional Modeling of the Structure of an Accretion Disk in a Binary System 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 Comparison Between Two- and Three-dimensional Modeling of the Structure of an Accretion Disk in a Binary System, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comparison Between Two- and Three-dimensional Modeling of the Structure of an Accretion Disk in a Binary System will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1525980