The formation pathways of compact elliptical galaxies
Abstract Compact elliptical (cE) galaxies remain an elusively difficult galaxy class to study. Recent observations have suggested that isolated and host-associated cEs have different formation pathways, while simulation studies have also shown different pathways can lead to a cE galaxy. However a so...
Published in: | Monthly Notices of the Royal Astronomical Society |
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croxfordunivpr:10.1093/mnras/stad2313 2023-08-27T04:11:48+02:00 The formation pathways of compact elliptical galaxies Deeley, Simon Drinkwater, Michael J Sweet, Sarah M Bekki, Kenji Couch, Warrick J Forbes, Duncan A 2023 http://dx.doi.org/10.1093/mnras/stad2313 https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad2313/51027614/stad2313.pdf en eng Oxford University Press (OUP) https://creativecommons.org/licenses/by/4.0/ Monthly Notices of the Royal Astronomical Society ISSN 0035-8711 1365-2966 Space and Planetary Science Astronomy and Astrophysics journal-article 2023 croxfordunivpr https://doi.org/10.1093/mnras/stad2313 2023-08-04T10:44:50Z Abstract Compact elliptical (cE) galaxies remain an elusively difficult galaxy class to study. Recent observations have suggested that isolated and host-associated cEs have different formation pathways, while simulation studies have also shown different pathways can lead to a cE galaxy. However a solid link has not been established, and the relative contributions of each pathway in a cosmological context remains unknown. Here we combine a spatially-resolved observational sample of cEs taken from the SAMI galaxy survey with a matched sample of galaxies within the IllustrisTNG cosmological simulation to establish an overall picture of how these galaxies form. The observed cEs located near a host galaxy appear redder, smaller and older than isolated cEs, supporting previous evidence for multiple formation pathways. Tracing the simulated cEs back through time, we find two main formation pathways; 32 ± 5 percent formed via the stripping of a spiral galaxy by a larger host galaxy, while 68 ± 4 percent formed through a gradual build-up of stellar mass in isolated environments. We confirm that cEs in different environments do indeed form via different pathways, with all isolated cEs in our sample having formed via in-situ formation (i.e. none were ejected from a previous host), and 77 ± 6 percent of host-associated cEs having formed via tidal stripping. Separating them by their formation pathway, we are able to reproduce the observed differences between isolated and host-associated cEs, showing that these differences can be fully explained by the different formation pathways dominating in each environment. Article in Journal/Newspaper sami Oxford University Press (via Crossref) Monthly Notices of the Royal Astronomical Society 525 1 1192 1209 |
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Oxford University Press (via Crossref) |
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Space and Planetary Science Astronomy and Astrophysics |
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Space and Planetary Science Astronomy and Astrophysics Deeley, Simon Drinkwater, Michael J Sweet, Sarah M Bekki, Kenji Couch, Warrick J Forbes, Duncan A The formation pathways of compact elliptical galaxies |
topic_facet |
Space and Planetary Science Astronomy and Astrophysics |
description |
Abstract Compact elliptical (cE) galaxies remain an elusively difficult galaxy class to study. Recent observations have suggested that isolated and host-associated cEs have different formation pathways, while simulation studies have also shown different pathways can lead to a cE galaxy. However a solid link has not been established, and the relative contributions of each pathway in a cosmological context remains unknown. Here we combine a spatially-resolved observational sample of cEs taken from the SAMI galaxy survey with a matched sample of galaxies within the IllustrisTNG cosmological simulation to establish an overall picture of how these galaxies form. The observed cEs located near a host galaxy appear redder, smaller and older than isolated cEs, supporting previous evidence for multiple formation pathways. Tracing the simulated cEs back through time, we find two main formation pathways; 32 ± 5 percent formed via the stripping of a spiral galaxy by a larger host galaxy, while 68 ± 4 percent formed through a gradual build-up of stellar mass in isolated environments. We confirm that cEs in different environments do indeed form via different pathways, with all isolated cEs in our sample having formed via in-situ formation (i.e. none were ejected from a previous host), and 77 ± 6 percent of host-associated cEs having formed via tidal stripping. Separating them by their formation pathway, we are able to reproduce the observed differences between isolated and host-associated cEs, showing that these differences can be fully explained by the different formation pathways dominating in each environment. |
format |
Article in Journal/Newspaper |
author |
Deeley, Simon Drinkwater, Michael J Sweet, Sarah M Bekki, Kenji Couch, Warrick J Forbes, Duncan A |
author_facet |
Deeley, Simon Drinkwater, Michael J Sweet, Sarah M Bekki, Kenji Couch, Warrick J Forbes, Duncan A |
author_sort |
Deeley, Simon |
title |
The formation pathways of compact elliptical galaxies |
title_short |
The formation pathways of compact elliptical galaxies |
title_full |
The formation pathways of compact elliptical galaxies |
title_fullStr |
The formation pathways of compact elliptical galaxies |
title_full_unstemmed |
The formation pathways of compact elliptical galaxies |
title_sort |
formation pathways of compact elliptical galaxies |
publisher |
Oxford University Press (OUP) |
publishDate |
2023 |
url |
http://dx.doi.org/10.1093/mnras/stad2313 https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad2313/51027614/stad2313.pdf |
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sami |
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sami |
op_source |
Monthly Notices of the Royal Astronomical Society ISSN 0035-8711 1365-2966 |
op_rights |
https://creativecommons.org/licenses/by/4.0/ |
op_doi |
https://doi.org/10.1093/mnras/stad2313 |
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Monthly Notices of the Royal Astronomical Society |
container_volume |
525 |
container_issue |
1 |
container_start_page |
1192 |
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1209 |
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1775355065612107776 |