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Distribution of Circumstellar Disk Masses in the Young Cluster NGC 2024

  • Authors: J. A. Eisner and John M. Carpenter

Eisner & Carpenter 2003 The Astrophysical Journal 598 1341.

  • Provider: AAS Journals

Caption: Fig. 3.

(a) NGC 2024, u‐﹩v﹩ coverage of the OVRO observations; (b) resultant beam after weighting the complete OVRO data set by using a robust parameter of 0.5; (c) OVRO beam only for u‐﹩v﹩ spacings greater than 20 kλ. The contour increments in (b) and (c) are 0.2. Positive contours are indicated by solid lines, and negative contours are indicated by dotted lines.

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