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Fig. 3

image

Comparisons of the millimeter images with the Subaru-HiCIAO near infrared polarization intensity images, for FU Ori (left), Z CMa (middle), and V1057 Cyg (right). In each panel, the angular resolution of the millimeter images are presented in bottom left. Left: the Subaru-HiCIAO H-band image (color), overplotted with the JVLA 33 GHz continuum image. Contours are 36 μJy beam−1 (10σ) × [1, 2, 3, 4, 5] (reproduced from Liu et al. 2017). Middle: the Subaru-HiCIAO K-band image (color), overplotted with the SMA 225 GHz continuum image. Contours are 5 mJy beam−1 (5σ) × [1, 2, 3, 4, 5, 6, 7]. The spatial offset between the millimeter emission peak and the coronagraphic mask can be casued by a combination of the astrometric uncertainty of SMA due to phase self-calibration, and the astrometric uncertainty of Subaru-HiCIAO. Right: the Subaru-HiCIAO H-band image (color), overplotted with the SMA 225 GHz continuum image. Contours are 0.72 mJy beam−1 (3σ) × [−1, 1, 3, 5, 7].

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