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Gemini-LIGHTS: Herbig Ae/Be and Massive T Tauri Protoplanetary Disks Imaged with Gemini Planet Imager

  • Authors: Evan A. Rich, John D. Monnier, Alicia Aarnio, Anna S. E. Laws, Benjamin R. Setterholm, David J. Wilner, Nuria Calvet, Tim Harries, Chris Miller, Claire L. Davies, Fred C. Adams, Sean M. Andrews, Jaehan Bae, Catherine Espaillat, Alexandra Z. Greenbaum, Sasha Hinkley, Stefan Kraus, Lee Hartmann, Andrea Isella, Melissa McClure, Rebecca Oppenheimer, Laura M. Pérez, Zhaohuan Zhu

Evan A. Rich et al 2022 The Astronomical Journal 164 .

  • Provider: AAS Journals

Caption: Figure 12.

Q ϕ and U ϕ images of targets that have previously been classified as FS CMa. The image scale is log and chosen to show target structure. See the figure set appearing on the online version of this work (Figure 2) for target specific color bars. The point sources in the FOV are labeled with a dashed black circle in Q ϕ images. The name of the target and the epoch in YYYYMMDD format can be found in the upper left of each image. The type of polarized image (Q ϕ or U ϕ ), the 1” scale and the size in au, and the photometry band (J or H) can be found along the bottom of each subimage. In U ϕ images, red is positive and blue is negative flux.

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