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dc.date.accessioned 2022-11-08T16:50:50Z
dc.date.available 2022-11-08T16:50:50Z
dc.date.issued 2009
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/145337
dc.description.abstract Schwarzschild's method to set up a model galaxy is most useful when the distribution in velocity space is unknown. Nevertheless, one has to know beforehand which kind of orbits are spawned by the potential of the model. Moreover, although the system thus generated is in equilibrium, it is not necessarily stable. Here, we present a new method that allows to build up a stable stellar system without any previous knowledge of its distribution in velocity space. en
dc.format.extent 369-369 es
dc.language en es
dc.subject methods: numerical es
dc.subject galaxies: kinematics and dynamics es
dc.title Building stable stellar systems with ρ as the only datum en
dc.type Articulo es
sedici.identifier.other doi:10.1017/s1743921309991347 es
sedici.identifier.issn 1743-9213 es
sedici.identifier.issn 1743-9221 es
sedici.creator.person Carpintero, Daniel Diego es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
mods.originInfo.place Instituto de Astrofísica de La Plata es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.event IAU Symposium 266 (Rio de Janeiro, Brazil, August 10-14, 2009) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 5, no. S266 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)