Are violent events responsible of a galaxy morphological loop?
- Autores
- Scannapieco, Cecilia; Smith Castelli, Analía Viviana; Tissera, Patricia Beatriz
- Año de publicación
- 2005
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We use cosmological SPH simulations to investigate the effects of mergers and interactions on the formation of the bulge and disc components of galactic systems. We find that secular evolution during mergers seems to be a key process in the formation of stable disc-bulge systems with observational counterparts and contributes to establish the fundamental relations observed in galaxies. Our findings suggest that the secular evolution phase couples the formation mechanisms of the bulge and disc components. According to our results, depending on the particular stability properties and merger parameters, violents events could drive a morphological loop in which the outcome could be a disc or a spheroid.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Galaxies: fundamental parameters
Galaxies: interactions
Methods: numerical - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/84822
Ver los metadatos del registro completo
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Are violent events responsible of a galaxy morphological loop?Scannapieco, CeciliaSmith Castelli, Analía VivianaTissera, Patricia BeatrizCiencias AstronómicasGalaxies: fundamental parametersGalaxies: interactionsMethods: numericalWe use cosmological SPH simulations to investigate the effects of mergers and interactions on the formation of the bulge and disc components of galactic systems. We find that secular evolution during mergers seems to be a key process in the formation of stable disc-bulge systems with observational counterparts and contributes to establish the fundamental relations observed in galaxies. Our findings suggest that the secular evolution phase couples the formation mechanisms of the bulge and disc components. According to our results, depending on the particular stability properties and merger parameters, violents events could drive a morphological loop in which the outcome could be a disc or a spheroid.Facultad de Ciencias Astronómicas y Geofísicas2005info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf261-262http://sedici.unlp.edu.ar/handle/10915/84822enginfo:eu-repo/semantics/altIdentifier/issn/1743-9213info:eu-repo/semantics/altIdentifier/doi/10.1017/S174392130500387Xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:16:14Zoai:sedici.unlp.edu.ar:10915/84822Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:15.322SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Are violent events responsible of a galaxy morphological loop? |
| title |
Are violent events responsible of a galaxy morphological loop? |
| spellingShingle |
Are violent events responsible of a galaxy morphological loop? Scannapieco, Cecilia Ciencias Astronómicas Galaxies: fundamental parameters Galaxies: interactions Methods: numerical |
| title_short |
Are violent events responsible of a galaxy morphological loop? |
| title_full |
Are violent events responsible of a galaxy morphological loop? |
| title_fullStr |
Are violent events responsible of a galaxy morphological loop? |
| title_full_unstemmed |
Are violent events responsible of a galaxy morphological loop? |
| title_sort |
Are violent events responsible of a galaxy morphological loop? |
| dc.creator.none.fl_str_mv |
Scannapieco, Cecilia Smith Castelli, Analía Viviana Tissera, Patricia Beatriz |
| author |
Scannapieco, Cecilia |
| author_facet |
Scannapieco, Cecilia Smith Castelli, Analía Viviana Tissera, Patricia Beatriz |
| author_role |
author |
| author2 |
Smith Castelli, Analía Viviana Tissera, Patricia Beatriz |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Galaxies: fundamental parameters Galaxies: interactions Methods: numerical |
| topic |
Ciencias Astronómicas Galaxies: fundamental parameters Galaxies: interactions Methods: numerical |
| dc.description.none.fl_txt_mv |
We use cosmological SPH simulations to investigate the effects of mergers and interactions on the formation of the bulge and disc components of galactic systems. We find that secular evolution during mergers seems to be a key process in the formation of stable disc-bulge systems with observational counterparts and contributes to establish the fundamental relations observed in galaxies. Our findings suggest that the secular evolution phase couples the formation mechanisms of the bulge and disc components. According to our results, depending on the particular stability properties and merger parameters, violents events could drive a morphological loop in which the outcome could be a disc or a spheroid. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
We use cosmological SPH simulations to investigate the effects of mergers and interactions on the formation of the bulge and disc components of galactic systems. We find that secular evolution during mergers seems to be a key process in the formation of stable disc-bulge systems with observational counterparts and contributes to establish the fundamental relations observed in galaxies. Our findings suggest that the secular evolution phase couples the formation mechanisms of the bulge and disc components. According to our results, depending on the particular stability properties and merger parameters, violents events could drive a morphological loop in which the outcome could be a disc or a spheroid. |
| publishDate |
2005 |
| dc.date.none.fl_str_mv |
2005 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
| dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/84822 |
| url |
http://sedici.unlp.edu.ar/handle/10915/84822 |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/issn/1743-9213 info:eu-repo/semantics/altIdentifier/doi/10.1017/S174392130500387X |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf 261-262 |
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