Three-dimensional, axisymmetric cusps without chaos
| dc.contributor.author | Sridhar, S. | |
| dc.contributor.author | Touma, Jihad R. | |
| dc.date.accessioned | 2012-07-11T06:00:57Z | |
| dc.date.available | 2012-07-11T06:00:57Z | |
| dc.date.issued | 1997 | |
| dc.description | Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations) | en |
| dc.description.abstract | We construct three-dimensional axisymmetric, cuspy density distributions, whose potentials are of Stackel form in parabolic coordinates. As in a recent paper by Sridhar BL Touma, a black hole of arbitrary mass may be added at the centre, without destroying the Stackel form of the potentials. The construction uses a classic method, originally owing to Kuzmin, which is extended to parabolic coordinates here. The models are highly oblate, and the cusps are 'weak', with the density, rho proportional to 1/r(k), where 0<k<1. | en |
| dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, 1997, Vol.292, p657 | en |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.uri | http://hdl.handle.net/2289/4859 | |
| dc.language.iso | en | en |
| dc.publisher | Blackwell Publishing for the Royal Astronomical Society | en |
| dc.relation.uri | http://adsabs.harvard.edu/abs/1997MNRAS.292..657S | en |
| dc.relation.uri | http://arxiv.org/abs/astro-ph/9704015 | en |
| dc.rights | 1997 Blackwell Publishing for the Royal Astronomical Society | en |
| dc.subject | galaxies | en |
| dc.subject | elliptical and lenticular | en |
| dc.title | Three-dimensional, axisymmetric cusps without chaos | en |
| dc.type | Article | en |