Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

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. 2.

Pointing positions for the OVRO mosaic (crosses), plotted over a K‐band image of the NGC 2024 cluster from Meyer (1996), showing the FWHM of the OVRO primary beam at the observed frequency (100 GHz; dotted circle ) and the unit gain contour of the map (solid curve).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions