Star formation in the intragroup medium and other diagnostics of the evolutionary stages of compact groups of galaxies
S. Torres-Flores, C. Mendes de Oliveira, D. F. de Mello, P. Amram, H., Plana, B. Epinat, J. Iglesias-Paramo

TL;DR
This study investigates star formation in the intragroup medium of seven compact galaxy groups, revealing that advanced evolutionary stages and HI clouds correlate with intergalactic star formation and the presence of young stellar objects.
Contribution
It provides new observational evidence linking group evolution stages and intragroup HI clouds to star formation outside galaxies in compact groups.
Findings
Evolved groups contain young blue objects < 100 Myr in intragroup medium.
Discovery of a tidal dwarf galaxy candidate in NGC 92.
Advanced group evolution correlates with intragroup star formation.
Abstract
Context: Compact groups of galaxies are entities that have high densities of galaxies and serve as laboratories to study galaxy interactions, intergalactic star formation and galaxy evolution. Aims: The main goal of this study is to search for young objects in the intragroup medium of seven compact groups of galaxies: HCG 2, 7, 22, 23, 92, 100 and NGC 92 as well as to evaluate the stage of interaction of each group. Methods: We used Fabry-Perot velocity fields and rotation curves together with GALEX NUV and FUV images and optical R-band and HI maps. Results: (i) HCG 7 and HCG 23 are in early stages of interaction, (ii) HCG 2 and HCG 22 are mildly interacting, and (iii) HCG 92, HCG 100 and NGC 92 are in late stages of evolution. We find that all three evolved groups contain populations of young blue objects in the intragroup medium, consistent with ages < 100 Myr, of which several…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
