Models of cuspy triaxial stellar systems. IV : rotating systems

Autores
Carpintero, Daniel Diego; Muzzio, Juan Carlos
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We built two self--consistent models of triaxial, cuspy, rotating stellar systemsadding rotation to non-rotating models presented in previous papers of thisseries. The final angular velocity of the material is not constant and varies withthe distance to the center and with the height over the equator of the systems,but the figure rotation is very uniform in both cases. Even though the additionof rotation to the models modifies their original semiaxes ratios, the finalrotating models are considerably flattened and triaxial. An analysis of theorbital content of the models shows that about two thirds of their orbits arechaotic but, nevertheless, the models are very stable over intervals of the orderof one Hubble time. The bulk of the regular orbits are short axis tubes, whilelong axis tubes are replaced by tubes whose axes lie on the short--long axesplane, but do not coincide with the major axis. Other types of regular orbitsthat do not appear in non--rotating systems, like horseshoes and orbits thatcross themselves, are also found in the present models. Finally, ourfrequency maps show empty regions where studies of orbits on fixed potentialsfound orbits, a likely consequence of the self--consistency of our models thatexcludes them.
Fil: Carpintero, Daniel Diego. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Muzzio, Juan Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Materia
Kinematics (galaxias)
Dynamics (galaxias)
Numerical methods
Chaos
Elliptical galaxies
Lenticular galaxies
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/35720
Acceder
id CONICETDig_8b808381e1882a8e614769243832acef
oai_identifier_str oai:ri.conicet.gov.ar:11336/35720
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Models of cuspy triaxial stellar systems. IV : rotating systemsCarpintero, Daniel DiegoMuzzio, Juan CarlosKinematics (galaxias)Dynamics (galaxias)Numerical methodsChaosElliptical galaxiesLenticular galaxieshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We built two self--consistent models of triaxial, cuspy, rotating stellar systemsadding rotation to non-rotating models presented in previous papers of thisseries. The final angular velocity of the material is not constant and varies withthe distance to the center and with the height over the equator of the systems,but the figure rotation is very uniform in both cases. Even though the additionof rotation to the models modifies their original semiaxes ratios, the finalrotating models are considerably flattened and triaxial. An analysis of theorbital content of the models shows that about two thirds of their orbits arechaotic but, nevertheless, the models are very stable over intervals of the orderof one Hubble time. The bulk of the regular orbits are short axis tubes, whilelong axis tubes are replaced by tubes whose axes lie on the short--long axesplane, but do not coincide with the major axis. Other types of regular orbitsthat do not appear in non--rotating systems, like horseshoes and orbits thatcross themselves, are also found in the present models. Finally, ourfrequency maps show empty regions where studies of orbits on fixed potentialsfound orbits, a likely consequence of the self--consistency of our models thatexcludes them.Fil: Carpintero, Daniel Diego. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Muzzio, Juan Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaWiley Blackwell Publishing, Inc2016-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/35720Carpintero, Daniel Diego; Muzzio, Juan Carlos; Models of cuspy triaxial stellar systems. IV : rotating systems; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 459; 3-2016; 1082-10960035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw720info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/459/1/1082/2609073?redirectedFrom=fulltextinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:30:24Zoai:ri.conicet.gov.ar:11336/35720instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:30:25.223CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Models of cuspy triaxial stellar systems. IV : rotating systems
title Models of cuspy triaxial stellar systems. IV : rotating systems
spellingShingle Models of cuspy triaxial stellar systems. IV : rotating systems
Carpintero, Daniel Diego
Kinematics (galaxias)
Dynamics (galaxias)
Numerical methods
Chaos
Elliptical galaxies
Lenticular galaxies
title_short Models of cuspy triaxial stellar systems. IV : rotating systems
title_full Models of cuspy triaxial stellar systems. IV : rotating systems
title_fullStr Models of cuspy triaxial stellar systems. IV : rotating systems
title_full_unstemmed Models of cuspy triaxial stellar systems. IV : rotating systems
title_sort Models of cuspy triaxial stellar systems. IV : rotating systems
dc.creator.none.fl_str_mv Carpintero, Daniel Diego
Muzzio, Juan Carlos
author Carpintero, Daniel Diego
author_facet Carpintero, Daniel Diego
Muzzio, Juan Carlos
author_role author
author2 Muzzio, Juan Carlos
author2_role author
dc.subject.none.fl_str_mv Kinematics (galaxias)
Dynamics (galaxias)
Numerical methods
Chaos
Elliptical galaxies
Lenticular galaxies
topic Kinematics (galaxias)
Dynamics (galaxias)
Numerical methods
Chaos
Elliptical galaxies
Lenticular galaxies
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We built two self--consistent models of triaxial, cuspy, rotating stellar systemsadding rotation to non-rotating models presented in previous papers of thisseries. The final angular velocity of the material is not constant and varies withthe distance to the center and with the height over the equator of the systems,but the figure rotation is very uniform in both cases. Even though the additionof rotation to the models modifies their original semiaxes ratios, the finalrotating models are considerably flattened and triaxial. An analysis of theorbital content of the models shows that about two thirds of their orbits arechaotic but, nevertheless, the models are very stable over intervals of the orderof one Hubble time. The bulk of the regular orbits are short axis tubes, whilelong axis tubes are replaced by tubes whose axes lie on the short--long axesplane, but do not coincide with the major axis. Other types of regular orbitsthat do not appear in non--rotating systems, like horseshoes and orbits thatcross themselves, are also found in the present models. Finally, ourfrequency maps show empty regions where studies of orbits on fixed potentialsfound orbits, a likely consequence of the self--consistency of our models thatexcludes them.
Fil: Carpintero, Daniel Diego. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Muzzio, Juan Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
description We built two self--consistent models of triaxial, cuspy, rotating stellar systemsadding rotation to non-rotating models presented in previous papers of thisseries. The final angular velocity of the material is not constant and varies withthe distance to the center and with the height over the equator of the systems,but the figure rotation is very uniform in both cases. Even though the additionof rotation to the models modifies their original semiaxes ratios, the finalrotating models are considerably flattened and triaxial. An analysis of theorbital content of the models shows that about two thirds of their orbits arechaotic but, nevertheless, the models are very stable over intervals of the orderof one Hubble time. The bulk of the regular orbits are short axis tubes, whilelong axis tubes are replaced by tubes whose axes lie on the short--long axesplane, but do not coincide with the major axis. Other types of regular orbitsthat do not appear in non--rotating systems, like horseshoes and orbits thatcross themselves, are also found in the present models. Finally, ourfrequency maps show empty regions where studies of orbits on fixed potentialsfound orbits, a likely consequence of the self--consistency of our models thatexcludes them.
publishDate 2016
dc.date.none.fl_str_mv 2016-03
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/35720
Carpintero, Daniel Diego; Muzzio, Juan Carlos; Models of cuspy triaxial stellar systems. IV : rotating systems; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 459; 3-2016; 1082-1096
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/35720
identifier_str_mv Carpintero, Daniel Diego; Muzzio, Juan Carlos; Models of cuspy triaxial stellar systems. IV : rotating systems; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 459; 3-2016; 1082-1096
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw720
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/459/1/1082/2609073?redirectedFrom=fulltext
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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