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Hints of a Population of Solar System Analog Planets from ALMA

  • Authors: Deryl E. Long, Ke Zhang, Richard Teague, and Edwin A. Bergin

2020 The Astrophysical Journal Letters 895 L46.

  • Provider: AAS Journals

Caption: Figure 3.

Our data image, model image, and residuals. For the data and model image, contour levels are in steps of [5, 10, 20, 30] × σ (where σ = 56 μJy beam−1, the rms of the image). For our residuals we plot contour levels [−7, −5, −4, −3, 3, 5] × σ (σ = 52 μJy beam−1). Negative values are dashed contours and positive values are solid.

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