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Measurement of Circumstellar Disk Sizes in the Upper Scorpius OB Association with ALMA

  • Authors: Scott A. Barenfeld, John M. Carpenter, Anneila I. Sargent, Andrea Isella, and Luca Ricci

2017 The Astrophysical Journal 851 85.

  • Provider: AAS Journals

Caption: Figure 1.

ALMA 0.88 mm observed, model, and residual images corresponding to the best-fit dust model parameters for each source. The real part of the deprojected visibilities for the observations (solid points) and best-fit model (solid curve) are also shown as a function of baseline length.

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