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Detection of Continuum Submillimeter Emission Associated with Candidate Protoplanets

  • Authors: Andrea Isella, Myriam Benisty, Richard Teague, Jaehan Bae, Miriam Keppler, Stefano Facchini, and Laura Pérez

2019 The Astrophysical Journal Letters 879 L25.

  • Provider: AAS Journals

Caption: Figure 8.

VLT/SPHERE NIR image (left panels; Müller et al. 2018) and VLT/MUSE Hα image (right panels; Haffert et al. 2019). The white contours are drawn at 3 and 5 times the rms noise level of the 855 μm continuum emission, imaged with robust = 0.3 (top row) and robust = 2 (bottom row). The signal located in the southwest of PDS 70 b in the VLT/MUSE image is likely due to instrumental artifacts (Haffert et al. 2019).

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