Statistics – Computation
Scientific paper
Nov 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...310..176l&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 310, Nov. 1, 1986, p. 176-188.
Statistics
Computation
122
Binary Stars, Star Formation, Stellar Evolution, Stellar Motions, Angular Momentum, Cross Sections, Polytropic Processes, Stellar Models, Stellar Rotation
Scientific paper
The cross sections for tidal capture binary formation are computed for polytropic models with indices n = 3/2, 2, and 3 to represent a wide range of stellar models. The computational procedure for the tidal capture cross sections is summarized, and the results of normal mode analyses and the capture cross sections are presented. It is estimated that 25 percent of the tidally captured binaries become mergers for a stellar system whose rms velocity is roughly 10 km/s (typical for globular clusters), while about 50 percent are expected to become mergers for rms velocity of roughly 300 km/s (typical for galactic nuclei). The implications of these results for the dynamical evolution of stellar systems influenced by tidally captured binaries are briefly discussed.
Lee Hyung Mok
Ostriker Jeremiah P.
No associations
LandOfFree
Cross sections for tidal capture binary formation and stellar merger 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 Cross sections for tidal capture binary formation and stellar merger, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cross sections for tidal capture binary formation and stellar merger will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1148735