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Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO

  • Authors: Camryn Mullin, Miles Lucas, Ruobing Dong, Jun Hashimoto, Haochang Jiang, Doug Johnstone, Kellen Lawson, Sean Brittain, Olivier Guyon, Tomoyuki Kudo, Julien Lozi, Joan Najita, He Sun, Motohide Tamura, Kevin Wagner

Camryn Mullin et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 11.

Polarization angle (left panel) and fraction (right panel) as a function of wavelength for the six nondetections. The star shapes indicate the mean values reported in Table 4. The dashed–dotted lines in the right panel indicate the theoretical maximum polarization percentage if polarization is purely ISM caused, as per Equation (8). HD 56895 and HD 148352 have reported extinctions of 0, and thus would have zero ISM polarization contribution.

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