Discovery of a protocluster core associated with an enormous Ly Nebula at
arXiv:2111.01384 · doi:10.3847/1538-4357/ac29c6
Abstract
The MAMMOTH-1 nebula at is an enormous Ly nebula (ELAN) extending to a 440 kpc scale at the center of the extreme galaxy overdensity BOSS 1441. In this paper, we present observations of the and 250 GHz dust-continuum emission from the MAMMOTH-1 using the IRAM NOrthern Extended Millimeter Array. Our observations show that emission in this ELAN has not extended widespread emission into the circum- and inter-galactic media. We also find a remarkable concentration of six massive galaxies in emission in the central 100 kpc region of the ELAN. Their velocity dispersions suggest a total halo mass of , marking a possible protocluster core associated with the ELAN. The peak position of the line emission from the obscured AGN is consistent with the location of the intensity peak of MAMMOTH-1 in the rest-frame UV band. Its luminosity line ratio between the and is 0.610.17. The other five galaxies have luminosities in the range of (2.1-7.1) K pc, with the star-formation rates derived from the 250GHz continuum of (36)-224 yr. Follow-up spectroscopic observations will further confirm more member galaxies and improve the accuracy of the halo mass estimation.
arXiv comment14 pages, 5 figures, 2 tables, accepted for publication in ApJ
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