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A JWST Project on 47 Tucanae. Overview, Photometry, and Early Spectroscopic Results of M Dwarfs and Observations of Brown Dwarfs

  • Authors: A. F. Marino, A. P. Milone, M. V. Legnardi, A. Renzini, E. Dondoglio, Y. Cavecchi, G. Cordoni, A. Dotter, E. P. Lagioia, T. Ziliotto, M. Bernizzoni, E. Bortolan, M. G. Carlos, S. Jang, A. Mohandasan, F. Muratore, M. Tailo

A. F. Marino et al 2024 The Astrophysical Journal 965 .

  • Provider: AAS Journals

Caption: Figure 2.

Left: proper motions for stars in field C brighter than m F322W2 = 24.0 mag. Stars in 47 Tucanae, within the red dotted circle, and SMC are clearly separated in this plot. Right: m F322W2 vs. m F110W − m F160W + m F115W − m F322W2 pseudo-CMD for probable cluster members (black circles), which are located within the red dotted circle in the left panel and for SMC stars (red crosses).

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