JWST reveals a possible galaxy merger in triply-lensed MACS0647JD
arXiv:2210.14123 · doi:10.3847/2041-8213/acc94b
Abstract
MACS0647JD is a triply-lensed galaxy originally discovered with the Hubble Space Telescope. Here we report new JWST imaging, which clearly resolves MACS0647JD as having two components that are either merging galaxies or stellar complexes within a single galaxy. Both are very small, with stellar masses and radii . The brighter larger component "A" is intrinsically very blue (), likely due to very recent star formation and no dust, and is spatially extended with an effective radius . The smaller component "B" appears redder (), likely because it is older () with mild dust extinction (), and a smaller radius . We identify galaxies with similar colors in a high-redshift simulation, finding their star formation histories to be out of phase. With an estimated stellar mass ratio of roughly 2:1 and physical projected separation , we may be witnessing a galaxy merger 400 million years after the Big Bang. We also identify a candidate companion galaxy C away, likely destined to merge with galaxies A and B. The combined light from galaxies A+B is magnified by factors of 8, 5, and 2 in three lensed images JD1, 2, and 3 with F356W fluxes , , (AB mag 25.1, 25.6, 26.6). MACS0647JD is significantly brighter than other galaxies recently discovered at similar redshifts with JWST. Without magnification, it would have AB mag 27.3 (). With a high confidence level, we obtain a photometric redshift of based on photometry measured in 6 NIRCam filters spanning , out to rest-frame. JWST NIRSpec observations planned for January 2023 will deliver a spectroscopic redshift and a more detailed study of the physical properties of MACS0647JD.
27 pages, 14 figures, accepted for publication in ApJL