Interaction Between a Slow Wind from AGB Star and a Jet in a Binary System

Details Interaction Between a Slow Wind from AGB Star and a Jet in a Binary System Interaction Between a Slow Wind from AGB Star and a Jet in a Binary System

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..313..190g&link_type=abstract

Asymmetrical Planetary Nebulae III: Winds, Structure and the Thunderbird, Proceedings of the conference held 28 July - 1 August

Astronomy and Astrophysics

Astronomy

Scientific paper

We present three-dimensional hydrodynamic simulations of the interaction between a slow wind from an asymptotic giant branch (AGB) star and a jet blown by an orbiting companion, which is assumed to originate from an accretion disk. Two distinct regimes in the wind-jet interaction are presented here. These are determinated by the ratio of the AGB wind to jet momentum flux.

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