Stagnation Knots in Precessing Jets

Details Stagnation Knots in Precessing Jets Stagnation Knots in Precessing Jets

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..13..123l&link_type=abstract

Emission Lines from Jet Flows, Isla Mujeres, Q.R., México, November 13-17, 2000 (Eds. W. J. Henney, W. Steffen, A. C. Raga, and

Astronomy and Astrophysics

Astronomy

Ism: Molecular Clouds, Ism: Shocks, Stars: Formation, Stars: Jets And Outflows

Scientific paper

The problem of the formation of a stagnation knot in the head of a precessing stellar jet is investigated from both an analytical and numerical point of view. This dense structure is formed via a similar method to that proposed by Steffen (these proceedings) for the formation of FLIERS in planetary nebulae. Initial results suggest that the formation of a stagnation knot is possibly an intrinsic instability in precessing jets

Affiliated with

Also associated with

No associations

Rating

Stagnation Knots in Precessing Jets 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 Stagnation Knots in Precessing Jets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stagnation Knots in Precessing Jets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1200389