Are violent events responsible of a galaxy morphological loop?

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 c...

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Detalles Bibliográficos
Autores principales: Scannapieco, Cecilia, Smith Castelli, Analía Viviana, Tissera, Patricia Beatriz
Formato: Articulo
Lenguaje:Inglés
Publicado: 2005
Materias:
Ciencias Astronómicas
Galaxies: fundamental parameters
Galaxies: interactions
Methods: numerical
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/84822
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-84822
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Galaxies: fundamental parameters
Galaxies: interactions
Methods: numerical
spellingShingle Ciencias Astronómicas
Galaxies: fundamental parameters
Galaxies: interactions
Methods: numerical
Scannapieco, Cecilia
Smith Castelli, Analía Viviana
Tissera, Patricia Beatriz
Are violent events responsible of a galaxy morphological loop?
topic_facet Ciencias Astronómicas
Galaxies: fundamental parameters
Galaxies: interactions
Methods: numerical
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.
format Articulo
Articulo
author Scannapieco, Cecilia
Smith Castelli, Analía Viviana
Tissera, Patricia Beatriz
author_facet Scannapieco, Cecilia
Smith Castelli, Analía Viviana
Tissera, Patricia Beatriz
author_sort Scannapieco, Cecilia
title Are violent events responsible of a galaxy morphological loop?
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?
publishDate 2005
url http://sedici.unlp.edu.ar/handle/10915/84822
work_keys_str_mv AT scannapiecocecilia areviolenteventsresponsibleofagalaxymorphologicalloop
AT smithcastellianaliaviviana areviolenteventsresponsibleofagalaxymorphologicalloop
AT tisserapatriciabeatriz areviolenteventsresponsibleofagalaxymorphologicalloop
bdutipo_str Repositorios
_version_ 1764820488619556864

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