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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2005
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v1_nC198_p261_Scannapieco http://hdl.handle.net/20.500.12110/paper_17439213_v1_nC198_p261_Scannapieco |
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paper:paper_17439213_v1_nC198_p261_Scannapieco2023-06-08T16:27:58Z Are violent events responsible of a galaxy morphological loop? Galaxies: fundamental parameters Galaxies: interactions Methods: numerical 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. © 2005 International Astronomical Union. 2005 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v1_nC198_p261_Scannapieco http://hdl.handle.net/20.500.12110/paper_17439213_v1_nC198_p261_Scannapieco |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
Galaxies: fundamental parameters Galaxies: interactions Methods: numerical |
| spellingShingle |
Galaxies: fundamental parameters Galaxies: interactions Methods: numerical Are violent events responsible of a galaxy morphological loop? |
| topic_facet |
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. © 2005 International Astronomical Union. |
| 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 |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v1_nC198_p261_Scannapieco http://hdl.handle.net/20.500.12110/paper_17439213_v1_nC198_p261_Scannapieco |
| _version_ |
1768545301926248448 |