Fission sequence and equilibrium models of rigidity rotating polytropes

Details Fission sequence and equilibrium models of rigidity rotating polytropes Fission sequence and equilibrium models of rigidity rotating polytropes

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..99...71h&link_type=abstract

(International Astronomical Union, Colloquium on Double Stars, Physical Properties and Generic Relations, 80th, Bandung, Indones

Astronomy and Astrophysics

Astrophysics

5

Binary Stars, Polytropic Processes, Stellar Evolution, Stellar Models, Angular Momentum, Angular Velocity, Equilibrium, Fission, Stellar Rotation

Scientific paper

Equilibrium sequences of self-gravitating and polytropic stars including
binary stars are computed for various polytropic indexes. The authors
find a fission sequence from an ellipsoidal configuration to a binary by
way of dumb-bell equilibrium.

Affiliated with

Also associated with

No associations

Rating

Fission sequence and equilibrium models of rigidity rotating polytropes 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 Fission sequence and equilibrium models of rigidity rotating polytropes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fission sequence and equilibrium models of rigidity rotating polytropes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1857374