On the relevance of chaos for halo stars in the solar neighbourhood
- Autores
- Maffione, Nicolás Pablo; Gómez, F.; Cincotta, Pablo Miguel; Giordano, Claudia Marcela; Cooper, Andrew P.; O'Shea, B.
- Año de publicación
- 2015
- Idioma
- español castellano
- Tipo de recurso
- artículo
- Estado
- versión aceptada
- Descripción
- Fil: Maffione, Nicolas P. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Maffione, Nicolás P. Instituto de Astrofísica de La Plata; Argentina.
Fil: Maffione, Nicolás P. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina
Fil: Gómez, F. Max-Planck-Institut fur Astrophysik; Alemania
Fil: Cincotta, Pablo M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina
Fil: Cincotta, Pablo M. Instituto de Astrofísica de La Plata; Argentina
Fil: Cincotta, Pablo M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Giordano, Claudia M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata; Argentina
Fil: Giordano, Claudia M. Instituto de Astrofísica de La Plata; Argentina.
Fil: Giordano, Claudia M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Cooper, A. University Of Durham; Reino Unido
Fil: O'Shea, B. Michigan State University; Estados Unidos
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. - Materia
-
Astronomía
Chaos
Diffusion
Methods
Numerical
Galaxy
Evolution
Astronomía - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de Río Negro
- OAI Identificador
- oai:rid.unrn.edu.ar:20.500.12049/2871
Ver los metadatos del registro completo
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On the relevance of chaos for halo stars in the solar neighbourhoodMaffione, Nicolás PabloGómez, F.Cincotta, Pablo MiguelGiordano, Claudia MarcelaCooper, Andrew P.O'Shea, B.AstronomíaChaosDiffusionMethodsNumericalGalaxyEvolutionAstronomíaFil: Maffione, Nicolas P. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Maffione, Nicolás P. Instituto de Astrofísica de La Plata; Argentina.Fil: Maffione, Nicolás P. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; ArgentinaFil: Gómez, F. Max-Planck-Institut fur Astrophysik; AlemaniaFil: Cincotta, Pablo M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; ArgentinaFil: Cincotta, Pablo M. Instituto de Astrofísica de La Plata; ArgentinaFil: Cincotta, Pablo M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Giordano, Claudia M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata; ArgentinaFil: Giordano, Claudia M. Instituto de Astrofísica de La Plata; Argentina.Fil: Giordano, Claudia M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Cooper, A. University Of Durham; Reino UnidoFil: O'Shea, B. Michigan State University; Estados UnidosWe 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.2015-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfMaffione, 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; 2830-28470035-8711https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stv1778 http://arxiv.org/abs/1508.00579 http://hdl.handle.net/11336/13886https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2871http://dx.doi.org/10.1093/mnras/stv1778spa453Monthly Notices of the Royal Astronomical Societyinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/4.0/reponame:RID-UNRN (UNRN)instname:Universidad Nacional de Río Negro2025-09-29T14:29:32Zoai:rid.unrn.edu.ar:20.500.12049/2871instacron:UNRNInstitucionalhttps://rid.unrn.edu.ar/jspui/Universidad públicaNo correspondehttps://rid.unrn.edu.ar/oai/snrdrid@unrn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:43692025-09-29 14:29:32.503RID-UNRN (UNRN) - Universidad Nacional de Río Negrofalse |
dc.title.none.fl_str_mv |
On the relevance of chaos for halo stars in the solar neighbourhood |
title |
On the relevance of chaos for halo stars in the solar neighbourhood |
spellingShingle |
On the relevance of chaos for halo stars in the solar neighbourhood Maffione, Nicolás Pablo Astronomía Chaos Diffusion Methods Numerical Galaxy Evolution Astronomía |
title_short |
On the relevance of chaos for halo stars in the solar neighbourhood |
title_full |
On the relevance of chaos for halo stars in the solar neighbourhood |
title_fullStr |
On the relevance of chaos for halo stars in the solar neighbourhood |
title_full_unstemmed |
On the relevance of chaos for halo stars in the solar neighbourhood |
title_sort |
On the relevance of chaos for halo stars in the solar neighbourhood |
dc.creator.none.fl_str_mv |
Maffione, Nicolás Pablo Gómez, F. Cincotta, Pablo Miguel Giordano, Claudia Marcela Cooper, Andrew P. O'Shea, B. |
author |
Maffione, Nicolás Pablo |
author_facet |
Maffione, Nicolás Pablo Gómez, F. Cincotta, Pablo Miguel Giordano, Claudia Marcela Cooper, Andrew P. O'Shea, B. |
author_role |
author |
author2 |
Gómez, F. Cincotta, Pablo Miguel Giordano, Claudia Marcela Cooper, Andrew P. O'Shea, B. |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Astronomía Chaos Diffusion Methods Numerical Galaxy Evolution Astronomía |
topic |
Astronomía Chaos Diffusion Methods Numerical Galaxy Evolution Astronomía |
dc.description.none.fl_txt_mv |
Fil: Maffione, Nicolas P. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Maffione, Nicolás P. Instituto de Astrofísica de La Plata; Argentina. Fil: Maffione, Nicolás P. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina Fil: Gómez, F. Max-Planck-Institut fur Astrophysik; Alemania Fil: Cincotta, Pablo M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina Fil: Cincotta, Pablo M. Instituto de Astrofísica de La Plata; Argentina Fil: Cincotta, Pablo M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Giordano, Claudia M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata; Argentina Fil: Giordano, Claudia M. Instituto de Astrofísica de La Plata; Argentina. Fil: Giordano, Claudia M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Cooper, A. University Of Durham; Reino Unido Fil: O'Shea, B. Michigan State University; Estados Unidos 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. |
description |
Fil: Maffione, Nicolas P. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina |
publishDate |
2015 |
dc.date.none.fl_str_mv |
2015-02 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/acceptedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
acceptedVersion |
dc.identifier.none.fl_str_mv |
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 0035-8711 https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stv1778 http://arxiv.org/abs/1508.00579 http://hdl.handle.net/11336/13886 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2871 http://dx.doi.org/10.1093/mnras/stv1778 |
identifier_str_mv |
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 0035-8711 |
url |
https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stv1778 http://arxiv.org/abs/1508.00579 http://hdl.handle.net/11336/13886 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2871 http://dx.doi.org/10.1093/mnras/stv1778 |
dc.language.none.fl_str_mv |
spa |
language |
spa |
dc.relation.none.fl_str_mv |
453 Monthly Notices of the Royal Astronomical Society |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/4.0/ |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/4.0/ |
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