Binary models of assymetric winds from late type stars

Details Binary models of assymetric winds from late type stars Binary models of assymetric winds from late type stars

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.7204m&link_type=abstract

American Astronomical Society, 188th AAS Meeting, #72.04; Bulletin of the American Astronomical Society, Vol. 28, p.944

Other

Scientific paper

One of the most plausible scenarios for the formation of asymmetric molecular envelopes from AGB stars and bipolar preplanetary nebulae, involves a mass losing red giant in the presence of a binary companion in a detached or common envelope configuration. The likelihood of the detached binary system scenario in the formation of asymmetric and bipolar flows is assessed by constructing 3-Dimensional Smooth Particle Hydrodynamic wind models. We investigate the effects of the binary companion, on an otherwise spherically symmetric dust-driven wind, as a function of the binary mass ratio and separation and we examine the importance of various heating and cooling mechanisms. We also produce models of outflows emanating from a tidally spun-up primary. In particular we examine whether appropriate conditions can arise that will allow the formation of an accretion disk around the secondary and of an exterior disk beyond the outer Lagrangian point of the system as proposed by Morris (1987,PASP,99,1115).

Affiliated with

Also associated with

No associations

Rating

Binary models of assymetric winds from late type stars 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 Binary models of assymetric winds from late type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Binary models of assymetric winds from late type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1355457