The range of core size of postcollapse clusters supported by primordial binaries

Details The range of core size of postcollapse clusters supported by primordial binaries The range of core size of postcollapse clusters supported by primordial binaries

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...431..231v&link_type=abstract

The Astrophysical Journal, Part 1, vol. 431, no. 1, p. 231-236

Statistics

Computation

35

Abundance, Binary Stars, Globular Clusters, Gravitational Collapse, Stellar Cores, Stellar Evolution, Astronomical Models, Celestial Mechanics, Computational Astrophysics, Protostars

Scientific paper

We investigate how the core size of globular clusters in a postcollapse
phase driven by primordial binaries depends upon the parameters of the
distribution of the binary binding energy and the abundance of the
binaries. We show that the variation of these quantites increases the
plausible range for the core size.

Affiliated with

Also associated with

No associations

Rating

The range of core size of postcollapse clusters supported by primordial 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 The range of core size of postcollapse clusters supported by primordial binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The range of core size of postcollapse clusters supported by primordial binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1494416