International Gemini Observatory/NOIRLab/NSF/AURA
Star Pair’s Dusty Disk Shines Light on Planet Formation
Left: J-band polarized intensity (P⊥) images. Right: P⊥ scaled by r2, where r is the distance in pixels from the central binary, corrected for projection effects. Both images are shown on a linear scale and oriented north up and east left. The coronagraph is represented by the black filled circles.
