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| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.provenance | Universidad Nacional de Río Negro | - |
| dc.creator | Maffione, Nicolas P. | - |
| dc.creator | Gómez, F. | - |
| dc.creator | Cincotta, Pablo M. | - |
| dc.creator | Giordano, Claudia M. | - |
| dc.creator | Cooper, A. | - |
| dc.creator | O'Shea, B. | - |
| dc.date | 2015-02 | - |
| dc.date.accessioned | 2020-02-11T14:09:14Z | - |
| dc.date.available | 2020-02-11T14:09:14Z | - |
| dc.date.issued | 2015-02 | - |
| dc.identifier | Maffione, Nicolas P., Gomez, F., Cincotta, Pablo M., Giordano, Claudia M., Cooper, A. & et al. (2015). On the relevance of chaos for halo stars in the solar neighbourhood. Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 453; 3; 2830-2847 | - |
| dc.identifier | 0035-8711 | - |
| dc.identifier | https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stv1778 | - |
| dc.identifier | http://arxiv.org/abs/1508.00579 | - |
| dc.identifier | http://hdl.handle.net/11336/13886 | - |
| dc.identifier | https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2871 | - |
| dc.identifier | http://dx.doi.org/10.1093/mnras/stv1778 | - |
| dc.identifier.uri | http://rodna.bn.gov.ar/jspui/handle/bnmm/575840 | - |
| dc.description | Fil: Maffione, Nicolas P. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina | - |
| dc.description | Fil: Maffione, Nicolas P. Instituto de Astrofísica de La Plata; Argentina. | - |
| dc.description | Fil: Maffione, Nicolas P. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina | - |
| dc.description | Fil: Gómez, F. Max-Planck-Institut fur Astrophysik; Alemania | - |
| dc.description | Fil: Cincotta, Pablo M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina | - |
| dc.description | Fil: Cincotta, Pablo M. Instituto de Astrofísica de La Plata; Argentina | - |
| dc.description | Fil: Cincotta, Pablo M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina | - |
| dc.description | Fil: Giordano, Claudia M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata; Argentina | - |
| dc.description | Fil: Giordano, Claudia M. Instituto de Astrofísica de La Plata; Argentina. | - |
| dc.description | Fil: Giordano, Claudia M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina | - |
| dc.description | Fil: Cooper, A. University Of Durham; Reino Unido | - |
| dc.description | Fil: O'Shea, B. Michigan State University; Estados Unidos | - |
| dc.description | We show that diffusion due to chaotic mixing in the neighbourhood of the Sun may not be as relevant as previously suggested in erasing phase space signatures of past Galactic accretion events. For this purpose, we analyse solar neighbourhood-like volumes extracted from cosmological simulations that naturally account for chaotic orbital behaviour induced by the strongly triaxial and cuspy shape of the resulting dark matter haloes, among other factors. In the approximation of an analytical static triaxial model, our results show that a large fraction of stellar halo particles in such local volumes have chaos onset times (i.e. the timescale at which stars commonly associated with chaotic orbits will exhibit their chaotic behaviour) significantly larger than a Hubble time. Furthermore, particles that do present a chaotic behaviour within a Hubble time do not exhibit significant diffusion in phase space. | - |
| dc.format | application/pdf | - |
| dc.language | spa | - |
| dc.relation | 453 | - |
| dc.relation | Monthly Notices of the Royal Astronomical Society | - |
| dc.rights | info:eu-repo/semantics/openAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/4.0/ | - |
| dc.source | reponame:RID-UNRN (UNRN) | - |
| dc.source | instname:Universidad Nacional de Río Negro | - |
| dc.source | instacron:UNRN | - |
| dc.source.uri | http://dx.doi.org/10.1093/mnras/stv1778 | - |
| dc.subject | Chaos | - |
| dc.subject | Diffusion | - |
| dc.subject | Methods | - |
| dc.subject | Numerical | - |
| dc.subject | Galaxy | - |
| dc.subject | Evolution | - |
| dc.subject | .::Ciencias Exactas y Naturales::Ciencias Físicas::Astronomía | - |
| dc.title | On the relevance of chaos for halo stars in the solar neighbourhood | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/acceptedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| dc.about | - | |
| Aparece en las colecciones: | Universidad Nacional de Río Negro | |
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