Numerical modeling of the evolution of unstable modes of jets from young stellar objects

Details Numerical modeling of the evolution of unstable modes of jets from young stellar objects Numerical modeling of the evolution of unstable modes of jets from young stellar objects

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007arep...51..985k&link_type=abstract

Astronomy Reports, Volume 51, Issue 12, pp.985-993

Astronomy and Astrophysics

Astronomy

95.30.Lz, 95.75.Pq, 97.21.+A

Scientific paper

We present the results of numerical simulations of radiating nodes in jets outflowing from young stellar objects. The development of the fundamental and first reflection harmonics of the jet during the essentially non-linear stage is considered. We have shown for the first time the possible formation of radiating nodes with diameters smaller than the jet cross section. We describe our numerical code, which makes it possible for this class of problem to maintain a stationary equilibrium in the radial coordinate and minimize the force imbalance resulting from the transfer of stationary distributions along the meridian coordinate in the computational grid.

Affiliated with

Also associated with

No associations

Rating

Numerical modeling of the evolution of unstable modes of jets from young stellar objects 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 Numerical modeling of the evolution of unstable modes of jets from young stellar objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical modeling of the evolution of unstable modes of jets from young stellar objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1527554