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The HI content of Hickson Compact Groups : J/A+A/670/A21

Authors :
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
Jones M.G.
Verdes-Montenegro, Lourdes
Moldon J.
Damas-Segovia A.
Borthakur S.
Luna S.
Yun M.S.
del Olmo A.
Perea J.
Cannon J.
Lopez Gutierrez D.
Cluver M.
Garrido, Julián
Sanchez, s
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
Jones M.G.
Verdes-Montenegro, Lourdes
Moldon J.
Damas-Segovia A.
Borthakur S.
Luna S.
Yun M.S.
del Olmo A.
Perea J.
Cannon J.
Lopez Gutierrez D.
Cluver M.
Garrido, Julián
Sanchez, s
Publication Year :
2023

Abstract

Hickson compact groups (HCGs) are dense configurations of four to ten galaxies, whose HI morphology appears to follow an evolutionary sequence of three phases, with gas initially confined to galaxies, then significant amounts spread throughout the intra-group medium, and finally with almost no gas remaining in the galaxies themselves. It has also been suggested that several groups may harbour a diffuse HI component that is resolved out by interferometric observations. The HI deficiency of HCGs is expected to increase as the HI morphological phase progresses along the evolutionary sequence. If this is the case, HI deficiency would be a rough proxy for the age and evolutionary state of a HCG. We aim to test this hypothesis for the first time using a large sample of HCGs and to investigate the evidence for diffuse HI in HCGs. We performed a uniform reduction of all publicly available VLA HI observations (38 HCGs) with a purpose-built pipeline that also maximises the reproducibility of this study. The resulting HI data cubes were then analysed with the latest software tools to perform a manual separation of emission features into those belonging to galaxies and those extending into the intra-group medium. We thereby classified the HI morphological phase of each group as well as quantified their HI deficiency compared to galaxies in isolation. We find little evidence that HI deficiency can be used as a proxy for the evolutionary phase of a compact group in either of the first two phases, with the distribution of HI deficiency being consistent in both. However, for the final phase, the distribution clearly shifts to high HI deficiencies, with more than 90% of the expected HI content typically missing. Across all HCGs studied, we identify a few cases where there is strong evidence for a diffuse gas component in the intra-group medium, which might be detectable with improved observations. We also classify a new sub-phase where groups contain a lone HI-bearing galaxy, but ar

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1442728558
Document Type :
Electronic Resource