Starburst galaxies in the Hydra i cluster
Artikel i vetenskaplig tidskrift, 2025
Studying the impact of environment on star formation and quenching pathways requires statistically relevant samples of galaxies in a wide mass range. We present a new catalog of 196 galaxies of the nearby Hydra I cluster out to ∼1.75r200, consisting of broad u,g,r,i,z along with narrowband Hα measurements. These deep optical images were obtained with the DECam camera (CTIO) and reach down to a surface brightness limit of μ(3σ 10″ × 10″) = 26.9 mag arcsec2 in the g band. We also report the HI properties for 89 cluster members detected with MeerKAT. A color magnitude diagram (CMD) shows a bimodal distribution typical of a cluster population, more evolved than those found in isolation. We combined optical Hα and WISE infrared data to compare the star formation history at two distinct timescales. Differences in the star-forming activity depicted by both populations manifest as a starburst in 24 found members. Of these, 18 starburst galaxies have neutral gas measurements, and they show disturbed HI disks that suggest an environmentally triggered boost in star formation within the last 107 yrs. Processes such as ram pressure stripping or tidal interactions may underlie their enhanced star-forming activity and asymmetric disks. Since Hydra s dynamical history is unclear, we examine the spatial and velocity distribution of the sample. We reveal a possible link between the large-scale structure feeding the Hydra I cluster and the heightened star-forming activity of the starburst galaxies. This feeding pattern matches the few substructures that have been identified in Hydra in previous works, and this may explain their origin. Our results portray a picture of a cluster with an evolved nature, plus a population of new infalling galaxies that manifest the impact of their first contact with the cluster environment through star formation, color, morphology, and gas content transformations.
Galaxies: interactions
Galaxies: starburst
Galaxies: evolution
Galaxies: star formation
Galaxies: clusters: general
Författare
C. C. De La Casa
Consejo Superior de Investigaciones Científicas (CSIC)
Kelley Michelle Hess
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
Consejo Superior de Investigaciones Científicas (CSIC)
Netherlands Institute for Radio Astronomy (ASTRON)
L. Verdes-Montenegro
Consejo Superior de Investigaciones Científicas (CSIC)
R. Kotulla
University of Wisconsin
Hao Chen
University of Cape Town
Zhejiang Lab
T. H. Jarrett
Western Sydney University
University of Hawaii
University of Cape Town
M. E. Cluver
Swinburne University of Technology
University of the Western Cape
Simon B. De Daniloff
Institut de Radioastronomie Millimétrique (IRAM)
Universidad de Granada
Marie Lou Gendron-Marsolais
Universite Laval
Consejo Superior de Investigaciones Científicas (CSIC)
C. Carignan
Université Joseph Ki-Zerbo
Université de Montréal
University of Cape Town
John S. Gallagher
University of Wisconsin
R. C. Kraan-Korteweg
University of Cape Town
R. Ianjamasimanana
Consejo Superior de Investigaciones Científicas (CSIC)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 704 A264Infrastruktur
Onsala rymdobservatorium
Ämneskategorier (SSIF 2025)
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/202553831