The Ly, CIV, and HeII nebulae around J1000+0234: a galaxy pair at the center of a galaxy overdensity at
arXiv:2210.07982 · doi:10.1093/mnras/stad594
Abstract
Ly 1216 (Ly) emission extending over around dusty, massive starbursts at might represent a short-lived phase in the evolution of present-day, massive quiescent galaxies. To obtain empirical constraints on this emerging scenario, we present Ly, CIV 1550 (CIV), and HeII 1640 (HeII) observations taken with the Multi Unit Spectroscopic Explorer towards J10000234: a galaxy pair at composed of a low-mass starburst (J10000234South) neighboring a massive Submillimeter Galaxy (SMG; J10000234North) that harbors a rotationally supported gas disk. Based on the spatial distribution and relative strength of Ly, CIV, and HeII, we find that star formation in J1000+0234South and an active galactic nucleus in J1000+0234North are dominant factors in driving the observed 40 kiloparsec-scale Ly blob (LAB). We use the non-resonant HeII line to infer kinematic information of the LAB. We find marginal evidence for two spatially and spectrally separated HeII regions, which suggests that the two-peaked Ly profile is mainly a result of two overlapping and likely interacting HI clouds. We also report the serendipitous identification of three Ly emitters spanning over a redshift bin (i.e., ) located at from J1000+0234. A galaxy overdensity analysis confirms that J1000+0234 lies near the center of a Megaparsec-scale galaxy overdensity at that might evolve into a galaxy cluster at . The properties of J1000+0234 and its large-scale environment strengthen the link between SMGs within LABs, tracing overdense regions, as the progenitors of local massive ellipticals in galaxy clusters.
arXiv commentAccepted for publication in MNRAS
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