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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. 5.

NGC 2024 star‐forming region, imaged in 3 mm continuum with the OVRO Millimeter Array (gray scale). This image is constructed from measurements with a u‐﹩v﹩ radius greater than 20 kλ, and the resultant angular resolution is 2﹩\farcs﹩53 × 2﹩\farcs﹩13. The unit gain contour is indicated by a solid line, and the average rms of the residuals within the unit gain contour is 0.75 mJy. The positions of near‐IR sources detected at K‐band (Meyer 1996) are indicated with open circles.

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