On the stream-accretion disk interaction - Response to increased mass transfer rate

Details On the stream-accretion disk interaction - Response to increased mass transfer rate On the stream-accretion disk interaction - Response to increased mass transfer rate

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336..350d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 336, Jan. 1, 1989, p. 350-359.

Astronomy and Astrophysics

Astrophysics

11

Accretion Disks, Astrophysics, Binary Stars, Dwarf Novae, Hydrodynamics, Mass Flow Rate, Flow Distribution, Gravitational Effects, Lagrangian Equilibrium Points, Viscosity

Scientific paper

The time-dependent interaction between the stream of mass from the inner Lagrangian point and the accretion disk, resulting from an increasing mass transfer rate is calculated. The calculation is fully three-dimensional, using a pseudoparticle description of the hydrodynamics. It is demonstrated that the results of such calculations, when combined with specific observations, have the potential of both determining essential parameters, such as the viscosity parameter alpha, and can distinguish between different models of dwarf nova eruptions.

Affiliated with

Also associated with

No associations

Rating

On the stream-accretion disk interaction - Response to increased mass transfer rate 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 stream-accretion disk interaction - Response to increased mass transfer rate, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the stream-accretion disk interaction - Response to increased mass transfer rate will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-825882