JWST MIRI observations reveal extended coronal [Ne V] and [Si VI] emission over 13-15 kpc and indicate that the southern nucleus J1356S likely hosts an obscured AGN, with the extended gas explained by photoionization from the northern quasar in low-density regions.
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Extended coronal line emission and new clues to a possible dual AGN in the merger J1356+1026
JWST MIRI observations reveal extended coronal [Ne V] and [Si VI] emission over 13-15 kpc and indicate that the southern nucleus J1356S likely hosts an obscured AGN, with the extended gas explained by photoionization from the northern quasar in low-density regions.