MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regions

Sorgho, Amidou et al.-- Full list of authors: Sorgho, A.; Verdes-Montenegro, L.; Ianjamasimanana, R.; Hess, K. M.; Jones, M. G.; Korsaga, M.; Wang, J.; Lin, X.; Solanes, J. M.; Cluver, M. E.; Cannon, J. M.; Bosma, A.; Athanassoula, E.; del Olmo, A.; Perea, J.; Moldón, J.; Wiegert, T.; Sanchez-Expósi...

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Autores: Sorgho, Amidou, Verdes-Montenegro, Lourdes, Ianjamasimanana, Roger, Hess, Kelley M., Korsaga, M., del Olmo, A., Perea, Jaime, Moldón, Javier, Wiegert, Theresa, Sánchez-Expósito, S., Garrido, Julián, García-Benito, Rubén, Pérez Jiménez, Enrique
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2025
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/390671
Acceso en línea:http://hdl.handle.net/10261/390671
Access Level:acceso abierto
Palabra clave:Galaxies: evolution
Galaxies: interactions
Intergalactic medium
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dc.title.none.fl_str_mv MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regions
title MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regions
spellingShingle MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regions
Sorgho, Amidou
Galaxies: evolution
Galaxies: interactions
Intergalactic medium
title_short MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regions
title_full MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regions
title_fullStr MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regions
title_full_unstemmed MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regions
title_sort MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regions
dc.creator.none.fl_str_mv Sorgho, Amidou
Verdes-Montenegro, Lourdes
Ianjamasimanana, Roger
Hess, Kelley M.
Korsaga, M.
del Olmo, A.
Perea, Jaime
Moldón, Javier
Wiegert, Theresa
Sánchez-Expósito, S.
Garrido, Julián
García-Benito, Rubén
Pérez Jiménez, Enrique
author Sorgho, Amidou
author_facet Sorgho, Amidou
Verdes-Montenegro, Lourdes
Ianjamasimanana, Roger
Hess, Kelley M.
Korsaga, M.
del Olmo, A.
Perea, Jaime
Moldón, Javier
Wiegert, Theresa
Sánchez-Expósito, S.
Garrido, Julián
García-Benito, Rubén
Pérez Jiménez, Enrique
author_role author
author2 Verdes-Montenegro, Lourdes
Ianjamasimanana, Roger
Hess, Kelley M.
Korsaga, M.
del Olmo, A.
Perea, Jaime
Moldón, Javier
Wiegert, Theresa
Sánchez-Expósito, S.
Garrido, Julián
García-Benito, Rubén
Pérez Jiménez, Enrique
author2_role author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Ministerio de Ciencia, Innovación y Universidades (España)
Junta de Andalucía
European Commission
Agencia Estatal de Investigación (España)
Australian Research Council
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Galaxies: evolution
Galaxies: interactions
Intergalactic medium
topic Galaxies: evolution
Galaxies: interactions
Intergalactic medium
description Sorgho, Amidou et al.-- Full list of authors: Sorgho, A.; Verdes-Montenegro, L.; Ianjamasimanana, R.; Hess, K. M.; Jones, M. G.; Korsaga, M.; Wang, J.; Lin, X.; Solanes, J. M.; Cluver, M. E.; Cannon, J. M.; Bosma, A.; Athanassoula, E.; del Olmo, A.; Perea, J.; Moldón, J.; Wiegert, T.; Sanchez-Expósito, S.; Garrido, J.; García-Benito, R.; Józsa, G. I. G.; Borthakur, S.; Jarrett, T.; Namumba, B.; Pérez, E.; Román, J.; Smirnov, O. M.; Yun, M.
publishDate 2025
dc.date.none.fl_str_mv 2025
2025
2025
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dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/390671
url http://hdl.handle.net/10261/390671
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spelling MeerKAT view of Hickson Compact Groups: II. HI deficiency in the cores and surrounding regionsSorgho, AmidouVerdes-Montenegro, LourdesIanjamasimanana, RogerHess, Kelley M.Korsaga, M.del Olmo, A.Perea, JaimeMoldón, JavierWiegert, TheresaSánchez-Expósito, S.Garrido, JuliánGarcía-Benito, RubénPérez Jiménez, EnriqueGalaxies: evolutionGalaxies: interactionsIntergalactic mediumSorgho, Amidou et al.-- Full list of authors: Sorgho, A.; Verdes-Montenegro, L.; Ianjamasimanana, R.; Hess, K. M.; Jones, M. G.; Korsaga, M.; Wang, J.; Lin, X.; Solanes, J. M.; Cluver, M. E.; Cannon, J. M.; Bosma, A.; Athanassoula, E.; del Olmo, A.; Perea, J.; Moldón, J.; Wiegert, T.; Sanchez-Expósito, S.; Garrido, J.; García-Benito, R.; Józsa, G. I. G.; Borthakur, S.; Jarrett, T.; Namumba, B.; Pérez, E.; Román, J.; Smirnov, O. M.; Yun, M.Context. Hickson compact groups (HCGs) offer an ideal environment for investigating galaxy transformation as a result of interactions. It has been established that the evolutionary sequence of HCGs is marked by an intermediate stage characterised by a substantial amount of H I in their intragroup medium (IGrM) in the form of tidal tails and bridges (phase 2), rapidly followed by a final stage in which no IGrM gas is found and i which their member galaxies are highly H I deficient (phase 3).Aims. Despite numerous single-dish and interferometric H I studies on the HCGs, a clear H I picture of the groups within their large-scale environment still remains to be uncovered. Taking advantage of MeerKAT’s high column density sensitivity and large field of view, we aim to investigate the rapid transformation of HCGs from the intermediate to late phases, and establish a picture of their gas content variations in the context of their large-scale environments.Methods. We performed MeerKAT observations of six HCGs that were selected to represent the intermediate and late phases of the proposed evolutionary sequence. Combining the H I observations with data from recent wide-field optical surveys, we evaluated the H I deficiencies of galaxies in a ∼30′ radius of the HCGs.Results. We find that galaxies surrounding both phases exhibit similar distributions in their gas content. Similarly, galaxies making up the cores of phase 2 HCGs are comparable to their neighbours in terms of H I deficiencies. However, phase 3 groups are over an order of magnitude more deficient than their surroundings, supporting previous findings that late-phase HCG galaxies are more evolved than their large-scale environments. ©The Authors 2025The MeerKAT telescope is operated by the South African Radio Astronomy Observatory (SARAO), which is a facility of the National Research Foundation, an agency of the Department of Science and Innovation. This work used the Spanish Prototype of an SRC (SPSRC, Garrido et al. 2021) service and support funded by the Ministerio de Ciencia, Innovación y Universidades (MICIU), by the Junta de Andalucía, by the European Regional Development Funds (ERDF) and by the European Union NextGenerationEU/PRTR. The SPSRC acknowledges financial support from the Agencia Estatal de Investigación (AEI) through the “Centre of Excellence Severo Ochoa” award to the Instituto de Astrofísica de Andalucía (IAA-CSIC) (SEV-2017-0709) and together with the authors AS, LVM, RI, KMH, RGB, AdO, JP, SSE, JG, BN JM, TW and EP from the grant CEX2021-001131-S funded by MICIU/AEI/10.13039/501100011033. AS, LVM, RI, JG, SSE and TW acknowledge financial support from the grant PID2021-123930OB-C21 funded by MICIU/AEI and by ERDF/EU. RI acknowledges financial support from grant TED2021-130231B-I00 funded by MICIU/AEI and by the European Union NextGeneration EU/PRTR. BN acknowledges financial support from the grant PTA2023-023268-I funded by MICIU/AEI. TW acknowledges financial support from the coordination of the participation in SKA-Spain, funded by MICIU. AdO and JP acknowledge further financial support from the MICIU through project PID2022-140871NB-C21 by ERDF/EU. R.G.B. acknowledges further financial support from grant PID2022-141755NB-I00. JM acknowledges financial support from grant PID2023-147883NB-C21, funded by MICIU/AEI/10.13039/501100011033. JMS acknowledges financial support from the Spanish state agency MICIU/AEI/10.13039/501100011033 and by ERDF/EU funds through research grant PID2022-140871NB-C22 and the additional support of MICIU/AEI/10.13039/501100011033 through the Centre of Excellence María de Maeztu’s award for the Institut de Ciències del Cosmos at the Universitat de Barcelona under contract CEX2019–000918–M. EA and AB acknowledge support from the Centre National d’Etudes Spatiales (CNES), France. MEC acknowledges the support of an Australian Research Council Future Fellowship (Project No. FT170100273) funded by the Australian Government. J.R. acknowledges financial support from the Spanish Ministry of Science and Innovation through the project PID2022-138896NB-C55. OMS’s research is supported by the South African Research Chairs Initiative of the Department of Science and Technology and National Research Foundation (grant No. 81737).With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (SEV-2017-0709).With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2021-001131-S).Peer reviewedEDP SciencesMinisterio de Ciencia, Innovación y Universidades (España)Junta de AndalucíaEuropean CommissionAgencia Estatal de Investigación (España)Australian Research CouncilConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202520252025info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/390671reponame:DIGITAL.CSIC. 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