Born at the same time?
The brightest galaxies of groups and clusters are extremely luminous galaxies, usually located in the centres of those systems – central galaxies. In the hierarchical scenario of structure formation, galaxies grow in mass and size by merging with their neighbours. Simulations predict that central ga...
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ftdatacite:10.5281/zenodo.2635377 2023-05-15T18:12:08+02:00 Born at the same time? Santucci, Giulia None 2019 https://dx.doi.org/10.5281/zenodo.2635377 https://zenodo.org/record/2635377 unknown Zenodo https://zenodo.org/communities/esoaus2019 https://dx.doi.org/10.5281/zenodo.2635376 https://zenodo.org/communities/esoaus2019 Open Access Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 info:eu-repo/semantics/openAccess CC-BY Text Poster article-journal ScholarlyArticle 2019 ftdatacite https://doi.org/10.5281/zenodo.2635377 https://doi.org/10.5281/zenodo.2635376 2021-11-05T12:55:41Z The brightest galaxies of groups and clusters are extremely luminous galaxies, usually located in the centres of those systems – central galaxies. In the hierarchical scenario of structure formation, galaxies grow in mass and size by merging with their neighbours. Simulations predict that central galaxies have higher merger rates than other similarly luminous early type galaxies, mostly due to their privileged position at the bottom of the gravitational potential of the cluster. The recent accretion history of galaxies can be read through their stellar population gradients. Therefore, central galaxies with active merger histories are predicted to have shallower metallicity gradients than satellite galaxies of a similar mass. We are examining the stellar population gradients (age and metallicity) of 445 central galaxies in the SAMI galaxy survey to determine whether they are offset from similarly massive satellite galaxies in order to reach a better understanding of their formation and evolution history. Still Image sami DataCite Metadata Store (German National Library of Science and Technology) |
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The brightest galaxies of groups and clusters are extremely luminous galaxies, usually located in the centres of those systems – central galaxies. In the hierarchical scenario of structure formation, galaxies grow in mass and size by merging with their neighbours. Simulations predict that central galaxies have higher merger rates than other similarly luminous early type galaxies, mostly due to their privileged position at the bottom of the gravitational potential of the cluster. The recent accretion history of galaxies can be read through their stellar population gradients. Therefore, central galaxies with active merger histories are predicted to have shallower metallicity gradients than satellite galaxies of a similar mass. We are examining the stellar population gradients (age and metallicity) of 445 central galaxies in the SAMI galaxy survey to determine whether they are offset from similarly massive satellite galaxies in order to reach a better understanding of their formation and evolution history. |
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Still Image |
author |
Santucci, Giulia None |
spellingShingle |
Santucci, Giulia None Born at the same time? |
author_facet |
Santucci, Giulia None |
author_sort |
Santucci, Giulia |
title |
Born at the same time? |
title_short |
Born at the same time? |
title_full |
Born at the same time? |
title_fullStr |
Born at the same time? |
title_full_unstemmed |
Born at the same time? |
title_sort |
born at the same time? |
publisher |
Zenodo |
publishDate |
2019 |
url |
https://dx.doi.org/10.5281/zenodo.2635377 https://zenodo.org/record/2635377 |
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sami |
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sami |
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https://zenodo.org/communities/esoaus2019 https://dx.doi.org/10.5281/zenodo.2635376 https://zenodo.org/communities/esoaus2019 |
op_rights |
Open Access Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 info:eu-repo/semantics/openAccess |
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CC-BY |
op_doi |
https://doi.org/10.5281/zenodo.2635377 https://doi.org/10.5281/zenodo.2635376 |
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