Statistics – Computation
Scientific paper
Jan 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...403..256h&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 403, no. 1, p. 256-270.
Statistics
Computation
24
Binary Stars, Computational Astrophysics, Star Clusters, Stellar Mass, Stellar Physics, Computerized Simulation, Resonance Scattering, Scattering Cross Sections, Stellar Models, Stellar Systems, Triple Stars
Scientific paper
Results of scattering experiments involving hard binaries with binding energies up to a few hundred times larger than the kinetic energy of the incoming field star are reported in the form of total and differential cross sections for a variety of processes. An accurate description of equal mass binary-single star scattering over a complete range of parameters is provided. The heating of star clusters through three-body processes, when stellar collisions can be ignored, as is the case for encounters involving degenerate stars, is illustrated by plotting the average amount of energy exchange between binaries and field stars as a function of binary hardness.
No associations
LandOfFree
Binary-single-star scattering. III - Numerical experiments for equal-mass hard binaries 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-single-star scattering. III - Numerical experiments for equal-mass hard binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Binary-single-star scattering. III - Numerical experiments for equal-mass hard binaries will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1776535