Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich halo
Published in Nature Astronomy
| Autores: | , , , , , , , , , , , , , , , , , , , , |
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| Tipo de documento: | artigo |
| Estado: | Versión aceptada para publicación |
| Data de publicação: | 2024 |
| País: | España |
| Recursos: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositório: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/407625 |
| Acesso em linha: | http://hdl.handle.net/10261/407625 http://arxiv.org/abs/2405.03744v3 |
| Access Level: | Acceso aberto |
| Palavra-chave: | astro-ph.GA astro-ph.CO |
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Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich halo |
| title |
Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich halo |
| spellingShingle |
Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich halo Pablo G. Pérez-González astro-ph.GA astro-ph.GA astro-ph.CO |
| title_short |
Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich halo |
| title_full |
Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich halo |
| title_fullStr |
Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich halo |
| title_full_unstemmed |
Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich halo |
| title_sort |
Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich halo |
| dc.creator.none.fl_str_mv |
Pablo G. Pérez-González Francesco D`Eugenio Bruno Rodríguez del Pino Hannah Übler Roberto Maiolino Santiago Arribas Giovanni Cresci Isabella Lamperti Andrew J. Bunker Stefano Carniani Stephane Charlot Christopher J. Willott Torsten Böker Eleonora Parlanti Jan Scholtz Giacomo Venturi Guillermo Barro Luca Costantin Ignacio Martín-Navarro James S. Dunlop Daniel Magee |
| author |
Pablo G. Pérez-González |
| author_facet |
Pablo G. Pérez-González Francesco D`Eugenio Bruno Rodríguez del Pino Hannah Übler Roberto Maiolino Santiago Arribas Giovanni Cresci Isabella Lamperti Andrew J. Bunker Stefano Carniani Stephane Charlot Christopher J. Willott Torsten Böker Eleonora Parlanti Jan Scholtz Giacomo Venturi Guillermo Barro Luca Costantin Ignacio Martín-Navarro James S. Dunlop Daniel Magee |
| author_role |
author |
| author2 |
Francesco D`Eugenio Bruno Rodríguez del Pino Hannah Übler Roberto Maiolino Santiago Arribas Giovanni Cresci Isabella Lamperti Andrew J. Bunker Stefano Carniani Stephane Charlot Christopher J. Willott Torsten Böker Eleonora Parlanti Jan Scholtz Giacomo Venturi Guillermo Barro Luca Costantin Ignacio Martín-Navarro James S. Dunlop Daniel Magee |
| author2_role |
author author author author author author author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
Ministerio de Ciencia e Innovación (España) Science and Technology Facilities Council (UK) European Research Council Royal Society (UK) Fundación la Caixa Pablo G. Pérez-González [0000-0003-4528-5639] Francesco D`Eugenio [0000-0003-2388-8172] Bruno Rodríguez del Pino [0000-0001-5171-3930] Roberto Maiolino [0000-0003-4891-0794] Santiago Arribas [0000-0002-4985-3819] Giovanni Cresci [0000-0001-7997-1640] Isabella Lamperti [0000-0002-5281-1417] Stefano Carniani [0000-0002-8651-9879] Stephane Charlot [0000-0002-6719-380X] Christopher J. Willott [0000-0003-3458-2275] Eleonora Parlanti [0000-0002-5666-7782] Jan Scholtz [0000-0002-7392-7814] Giacomo Venturi [0000-0001-6010-6809] Guillermo Barro [0000-0001-8349-3055] Luca Costantin [0000-0001-6820-0015] Ignacio Martín-Navarro [0000-0001-8494-0080] Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
astro-ph.GA astro-ph.GA astro-ph.CO |
| topic |
astro-ph.GA astro-ph.GA astro-ph.CO |
| description |
Published in Nature Astronomy |
| publishDate |
2024 |
| dc.date.none.fl_str_mv |
2024 2025 2025 |
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info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Postprint info:eu-repo/semantics/acceptedVersion |
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article |
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acceptedVersion |
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http://hdl.handle.net/10261/407625 http://arxiv.org/abs/2405.03744v3 |
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http://hdl.handle.net/10261/407625 http://arxiv.org/abs/2405.03744v3 |
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Inglés |
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Inglés |
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https://doi.org/10.1038/s41550-025-02586-8 Sí |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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Springer Nature |
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Springer Nature |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim4$ gas-rich haloPablo G. Pérez-GonzálezFrancesco D`EugenioBruno Rodríguez del PinoHannah ÜblerRoberto MaiolinoSantiago ArribasGiovanni CresciIsabella LampertiAndrew J. BunkerStefano CarnianiStephane CharlotChristopher J. WillottTorsten BökerEleonora ParlantiJan ScholtzGiacomo VenturiGuillermo BarroLuca CostantinIgnacio Martín-NavarroJames S. DunlopDaniel Mageeastro-ph.GAastro-ph.GAastro-ph.COPublished in Nature AstronomyStars in galaxies form when baryons radiatively cool down and fall into gravitational wells whose mass is dominated by dark matter. Eventually, star formation quenches as gas is depleted and/or perturbed by feedback processes, no longer being able to collapse and condense. We report the first spatially resolved spectroscopic observations, using the JWST/NIRSpec IFU, of a massive, completely quiescent galaxy (Jekyll) and its neighborhood at $z=3.714$, when the Universe age was 10% of today's. Jekyll resides in a massive dark matter halo (with mass M$_\mathrm{DM}>10^{12}$ M$_\odot$) and forms a galaxy pair with Hyde, which shows very intense dust-enshrouded star formation (star formation rate $\sim300$ M$_\odot$yr$^{-1}$). We find large amounts of kinematically perturbed ionized and neutral gas in the circumgalactic medium around the pair. Despite this large gas reservoir, Jekyll, which formed $10^{11}$ M$_\odot$ in stars and chemically enriched early (first billion years of the Universe) and quickly (200-300 Myr), has remained quiescent for over 500 Myr. The properties of the gas found around the two galaxies are consistent with intense, AGN-induced photoionization, or intense shocks. However, with the current data no obscured or unobscured AGN is detected in the central galaxy (Jekyll) nor in the very active and dust rich star-forming galaxy (Hyde).We thank K. Glazebrook, who discovered the Jekyll galaxy, for his input on the nature of the system that improved this paper, and E. Bertola for their useful comments on the paper. We thank G. Mazzolari for helping with the analysis of the radio data. We acknowledge support from grants PID2022-139567NB-I00, PID2021-127718NB-I00 and PID2022-140483NB-C22 funded by Spanish Ministerio de Ciencia e Innovación MCIN/AEI/10.13039/501100011033, FEDER Una manera de hacer Europa, the Recovery, Transformation and resilience Plan from the Spanish State, and by NextGenerationEU from the European Union through the Recovery and Resilience Facility, and the Ramón y Cajal grant RYC2023-044853-I. We are grateful for the support of the ALMA EU archive. The project leading to this publication has received support from ORP, which is funded by the European Union’s Horizon 2020 research and innovation programme under grant agreement number 101004719 [ORP]. F.D’E., R.M. and J.S. acknowledge support by the Science and Technology Facilities Council (STFC), by the ERC through Advanced Grant 695671 ‘QUENCH’, and by the UKRI Frontier Research grant RISEandFALL. F.D’E. is grateful to C. Conroy for sharing the high-resolution C3K/MIST library. R.M. also acknowledges funding from a research professorship from the Royal Society. H.Ü. acknowledges funding by the European Union (ERC APEX, 101164796). Views and opinions expressed are however those of the authors only and do not necessarily reflect those of the European Union or the European Research Council Executive Agency. Neither the European Union nor the granting authority can be held responsible for them. A.J.B. acknowledges funding from the ‘FirstGalaxies’ Advanced Grant from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement number 789056). S. Carniani, E.P. and G.V. acknowledge support by European Union’s HE ERC Starting Grant number 101040227 - WINGS. G.C. acknowledges the support of the INAF Large Grant 2022 ‘The metal circle: a new sharp view of the baryon cycle up to Cosmic Dawn with the latest generation IFU facilities’. The project that gave rise to these results received the support of a fellowship from the “la Caixa” Foundation (ID 100010434) awarded to L.C.; the fellowship code is LCF/BQ/PR24/12050015. I.L. acknowledges support from PRIN-MUR project “PROMETEUS” financed by the European Union - Next Generation EU, Mission 4 Component 1 CUP B53D23004750006Peer reviewedSpringer NatureMinisterio de Ciencia e Innovación (España)Science and Technology Facilities Council (UK)European Research CouncilRoyal Society (UK)Fundación la CaixaPablo G. Pérez-González [0000-0003-4528-5639]Francesco D`Eugenio [0000-0003-2388-8172]Bruno Rodríguez del Pino [0000-0001-5171-3930]Roberto Maiolino [0000-0003-4891-0794]Santiago Arribas [0000-0002-4985-3819]Giovanni Cresci [0000-0001-7997-1640]Isabella Lamperti [0000-0002-5281-1417]Stefano Carniani [0000-0002-8651-9879]Stephane Charlot [0000-0002-6719-380X]Christopher J. Willott [0000-0003-3458-2275]Eleonora Parlanti [0000-0002-5666-7782]Jan Scholtz [0000-0002-7392-7814]Giacomo Venturi [0000-0001-6010-6809]Guillermo Barro [0000-0001-8349-3055]Luca Costantin [0000-0001-6820-0015]Ignacio Martín-Navarro [0000-0001-8494-0080]Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202520252024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Postprintinfo:eu-repo/semantics/acceptedVersionapplication/pdfhttp://hdl.handle.net/10261/407625http://arxiv.org/abs/2405.03744v3reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttps://doi.org/10.1038/s41550-025-02586-8Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/4076252026-05-22T06:33:51Z |
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15,81155 |