A merging pair of massive quiescent galaxies at <i>z</i> = 3.44 in the Cosmic Vine
We report the spectroscopic confirmation of a merging pair of massive quiescent galaxies at z = 3.44. Using JWST observations, we confirm that the two galaxies lie at a projected separation of 4.5 kpc with a velocity offset of ∼680 km s −1 ( δ z ∼ 0.01). The pair resides in the core of a known rich overdensity of galaxies, dubbed the “Cosmic Vine”. For both pair members, modeling of the spectral energy distributions and faint rest-frame optical emission lines indicate high stellar masses (log( M ⋆ / M ⊙ ) ∼ 10.9) and suppressed star formation (log(sSFR/yr −1 ) < −10), more than an order of magnitude below the level of the star formation main sequence at this redshift. We then explore the Illustris-TNG simulation and the GAEA and SHARK semi-analytical models to examine whether they produce a pair of massive quiescent galaxies akin to that of the Cosmic Vine. While all models produce close pairs of massive quiescent galaxies at 2 < z < 4 with comparable separations and velocity offsets, their predicted number densities are 10–80 times lower than our observational constraint. This discrepancy cannot be fully explained by coarse time sampling in these models or the general challenge of forming early massive quiescent galaxies in simulations. Given that > 90% of simulated pairs in the models that we analyzed merge by z = 0, our findings suggest that our observed pair will likely coalesce into a single massive galaxy. The merger, occurring in the dense core of a large-scale structure, might represent a critical event in the formation of a brightest cluster galaxy and the morphological transformation of high-redshift disky quiescent galaxies into early-type ellipticals.
Authors
- Masato Onodera (ORCID: https://orcid.org/0000-0003-3228-7264)
- R. Shimakawa
- Peifei Zhu (ORCID: https://orcid.org/0000-0001-7783-8811)
- M. L. Hamadouche (ORCID: https://orcid.org/0000-0001-6763-5551)
- Francesco Valentino (ORCID: https://orcid.org/0000-0001-6477-4011)
- C. D. P. Lagos
- Mariko Kubo (ORCID: https://orcid.org/0000-0002-7598-5292)
- David Blánquez-Sesé (ORCID: https://orcid.org/0000-0001-7880-8841)
- G. Brammer
- M. Tanaka
- Fabio Fontanot (ORCID: https://orcid.org/0000-0003-4744-0188)
- Marion Farcy (ORCID: https://orcid.org/0000-0002-5228-2244)
- M. Hirschmann
- Francesca Rizzo (ORCID: https://orcid.org/0000-0001-9705-2461)
- G. Magdis (ORCID: https://orcid.org/0000-0002-4872-2294)
- Lizhi Xie (ORCID: https://orcid.org/0000-0003-3864-068X)
- S. Jin
- Daniel Ceverino (ORCID: https://orcid.org/0000-0002-8680-248X)
- Christian Kragh Jespersen (ORCID: https://orcid.org/0000-0002-8896-6496)
- Steven Gillman (ORCID: https://orcid.org/0000-0001-9885-4589)
- Sune Toft (ORCID: https://orcid.org/0000-0003-3631-7176)
- K. E. Heintz (ORCID: https://orcid.org/0000-0002-9389-7413)
- Andreas L. Faisst (ORCID: https://orcid.org/0000-0002-9382-9832)
- Kei Ito (ORCID: https://orcid.org/0000-0002-9453-0381)
- Anna de Graaff (ORCID: https://orcid.org/0000-0002-2380-9801)
- Minju Lee (ORCID: https://orcid.org/0000-0002-2419-3068)
- G de Lucia (ORCID: https://orcid.org/0000-0003-2219-1250)
- K Whitaker
- A Manchester Man
Institutions
- Damien Foundation (BD)
Publication Details
- Journal
- Astronomy and Astrophysics
- Published
- 2025-04-03
- DOI
- https://doi.org/10.1051/0004-6361/202453211
- Citations
- 12
- Primary Topic
- Astronomy and Astrophysical Research
- Type
- article
- Field-Weighted Citation Impact
- 14.30
Funders
- National Science Foundation
- Ministerio de Ciencia, Innovación y Universidades
- National Research Foundation
- Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
- Danmarks Grundforskningsfond
- European Southern Observatory
- Natural Sciences and Engineering Research Council of Canada
- Japan Society for the Promotion of Science