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On the generalized Schuster density law
Author(s) -
S. Ninković
Publication year - 1998
Publication title -
serbian astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.196
H-Index - 16
eISSN - 1820-9289
pISSN - 1450-698X
DOI - 10.2298/saj9858015n
Subject(s) - physics , galaxy , radius , distribution (mathematics) , astrophysics , mass distribution , exponent , circular symmetry , symmetry (geometry) , stellar mass , mathematical physics , spiral galaxy , halo , exponential function , law , classical mechanics , mathematical analysis , star formation , geometry , linguistics , philosophy , computer security , mathematics , computer science , political science
A special case of the generalized Schuster density law for stellar systems with spherical symmetry is discussed; here the exponent in the denominator is equal to i/2 where i is a positive integer. Special attention is paid to the situation 2 ≤ i ≤ 5 since then the mass distributions in almost all approximately spherical stellar systems and subsystems known to exist - e. g. dark coronae of galaxies, bulges and halos of spiral galaxies, as well as the systems with the classical Schuster density law - are included. With certain improvements one can also obtain more ample variants including the density continuously attaining zero at a finite radius, somewhat different descriptions of the mass distribution, as well as generalizations towards axial symmetry. It is shown among others, that a spheroid with this mass distribution (i=4) yields the same total mass as the exponential disc and that the mass distribution proposed by King belongs asymptotically to the generalized Schuster density law (i=3)

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