On the Origin of Star Formation Quenching of Galaxies in Group Environments using the NewHorizon simulation Article Swipe
Jinsu Rhee
,
Sukyoung K. Yi
,
Jongwan Ko
,
Emanuele Contini
,
J. K. Jang
,
Seyoung Jeon
,
San Han
,
Christophe Pichon
,
Yohan Dubois
,
Katarina Kraljic
,
Sébastien Peirani
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2408.08353
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2408.08353
We study star formation (SF) quenching of satellite galaxies with $M_{*} > 10^7\,M_{\odot}$ within two low-mass groups ($M_{\rm vir}=10^{12.9}$ and $10^{12.7} \,M_{\odot}$) using the NewHorizon simulation. We confirm that satellite galaxies ($M_{*}\lesssim10^{10}\,M_{\odot}$) are more prone to quenching than their field counterparts. This quenched fraction decreases with increasing stellar mass, consistent with recent studies. Similar to the findings in cluster environments, we note a correlation between the orbital motions of galaxies within these groups and the phenomenon of SF quenching. Specifically, SF is suppressed at the group center, and for galaxies with $M_{*} > 10^{9.1}\,M_{\odot}$, there is often a notable rejuvenation phase following a temporary quenching period. The SF quenching at the group center is primarily driven by changes in star formation efficiency and the amount of gas available, both of which are influenced by hydrodynamic interactions between the interstellar medium and surrounding hot gas within the group. Conversely, satellite galaxies with $M_{*} < 10^{8.2}\,M_{\odot}$ experience significant gas removal within the group, leading to SF quenching. Our analysis highlights the complexity of SF quenching in satellite galaxies in group environments, which involves an intricate competition between the efficiency of star formation (which depends on the dynamical state of the gas) on the one hand, and the availability of cold dense gas on the other hand. This challenges the typical understanding of environmental effects based on gas stripping through ram pressure, suggesting a need for a new description of galaxy evolution under mild environmental effects.
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Metadata
- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2408.08353
- https://arxiv.org/pdf/2408.08353
- OA Status
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- Related Works
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- OpenAlex ID
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All OpenAlex metadata
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- DOI
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https://doi.org/10.48550/arxiv.2408.08353Digital Object Identifier
- Title
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On the Origin of Star Formation Quenching of Galaxies in Group Environments using the NewHorizon simulationWork title
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preprintOpenAlex work type
- Language
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enPrimary language
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2024Year of publication
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2024-08-15Full publication date if available
- Authors
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Jinsu Rhee, Sukyoung K. Yi, Jongwan Ko, Emanuele Contini, J. K. Jang, Seyoung Jeon, San Han, Christophe Pichon, Yohan Dubois, Katarina Kraljic, Sébastien PeiraniList of authors in order
- Landing page
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https://arxiv.org/abs/2408.08353Publisher landing page
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https://arxiv.org/pdf/2408.08353Direct link to full text PDF
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YesWhether a free full text is available
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greenOpen access status per OpenAlex
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https://arxiv.org/pdf/2408.08353Direct OA link when available
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Star formation, Galaxy, Group (periodic table), Quenching (fluorescence), Astrophysics, Star (game theory), Galaxy group, Physics, Galaxy formation and evolution, Quantum mechanics, FluorescenceTop concepts (fields/topics) attached by OpenAlex
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0Total citation count in OpenAlex
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| abstract_inverted_index.($M_{\rm | 17 |
| abstract_inverted_index.analysis | 166 |
| abstract_inverted_index.effects. | 242 |
| abstract_inverted_index.findings | 56 |
| abstract_inverted_index.fraction | 43 |
| abstract_inverted_index.galaxies | 8, 30, 69, 89, 149, 175 |
| abstract_inverted_index.involves | 180 |
| abstract_inverted_index.low-mass | 15 |
| abstract_inverted_index.quenched | 42 |
| abstract_inverted_index.studies. | 52 |
| abstract_inverted_index.decreases | 44 |
| abstract_inverted_index.dynamical | 194 |
| abstract_inverted_index.evolution | 238 |
| abstract_inverted_index.following | 101 |
| abstract_inverted_index.formation | 3, 120, 189 |
| abstract_inverted_index.intricate | 182 |
| abstract_inverted_index.pressure, | 228 |
| abstract_inverted_index.primarily | 114 |
| abstract_inverted_index.quenching | 5, 36, 104, 108, 172 |
| abstract_inverted_index.satellite | 7, 29, 148, 174 |
| abstract_inverted_index.stripping | 225 |
| abstract_inverted_index.temporary | 103 |
| abstract_inverted_index.$10^{12.7} | 20 |
| abstract_inverted_index.NewHorizon | 24 |
| abstract_inverted_index.available, | 127 |
| abstract_inverted_index.challenges | 215 |
| abstract_inverted_index.complexity | 169 |
| abstract_inverted_index.consistent | 49 |
| abstract_inverted_index.efficiency | 121, 186 |
| abstract_inverted_index.experience | 154 |
| abstract_inverted_index.highlights | 167 |
| abstract_inverted_index.increasing | 46 |
| abstract_inverted_index.influenced | 132 |
| abstract_inverted_index.phenomenon | 75 |
| abstract_inverted_index.quenching. | 78, 164 |
| abstract_inverted_index.suggesting | 229 |
| abstract_inverted_index.suppressed | 82 |
| abstract_inverted_index.Conversely, | 147 |
| abstract_inverted_index.competition | 183 |
| abstract_inverted_index.correlation | 63 |
| abstract_inverted_index.description | 235 |
| abstract_inverted_index.significant | 155 |
| abstract_inverted_index.simulation. | 25 |
| abstract_inverted_index.surrounding | 141 |
| abstract_inverted_index.availability | 205 |
| abstract_inverted_index.hydrodynamic | 134 |
| abstract_inverted_index.interactions | 135 |
| abstract_inverted_index.interstellar | 138 |
| abstract_inverted_index.rejuvenation | 99 |
| abstract_inverted_index.Specifically, | 79 |
| abstract_inverted_index.\,M_{\odot}$) | 21 |
| abstract_inverted_index.counterparts. | 40 |
| abstract_inverted_index.environmental | 220, 241 |
| abstract_inverted_index.environments, | 59, 178 |
| abstract_inverted_index.understanding | 218 |
| abstract_inverted_index.vir}=10^{12.9}$ | 18 |
| abstract_inverted_index.10^7\,M_{\odot}$ | 12 |
| abstract_inverted_index.10^{8.2}\,M_{\odot}$ | 153 |
| abstract_inverted_index.10^{9.1}\,M_{\odot}$, | 93 |
| abstract_inverted_index.($M_{*}\lesssim10^{10}\,M_{\odot}$) | 31 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 11 |
| citation_normalized_percentile |