Other
Scientific paper
Nov 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994babel.150....7n&link_type=abstract
Bulletin Astronomique de Belgrade, No. 150, p. 7 - 10
Other
Stellar Systems: Energies
Scientific paper
The case of spherically symmetric, self-consistent, stellar systems, whose total mass is contained within a finite radius, is considered. A general formula for their potential energy, where the latter is expressed in terms of the total-mass square, limiting radius and a dimensionless coefficient depending on the general density slope, is given. Though the increase of this dimensionless coefficient follows the increasing in another dimensionless quantity (ratio limiting radius to half-mass one), the ratio of the two, for the case of the realistic models examined in the present paper, remains almost constant, usually about 0.4 - 0.5 depending on the given model.
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