Image Details

Choose export citation format:

The Open Cluster Chemical Abundances and Mapping Survey. VIII. Galactic Chemical Gradient and Azimuthal Analysis from SDSS/MWM DR19

  • Authors: Jonah M. Otto, Peter M. Frinchaboy, Natalie R. Myers, James W. Johnson, John Donor, Ahabar Hossain, Szabolcs Mészáros, Hailey Wallace, Katia Cunha, Binod Bhattarai, Amaya Sinha, Gail Zasowski, Sarah R. Loebman, Alessa I. Wiggins, Adrian M. Price-Whelan, Taylor Spoo, Diogo Souto, Dmitry Bizyaev, Kaike Pan, Andrew K. Saydjari, Ying-Yi Song

Jonah M. Otto et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 8.

Same plot as Figure 2, where the entire cluster sample is plotted in XY space, colored by the mean [Fe/H] abundance. The diamond points denote clusters that were in OCCAM DR17/N. Myers et al. (2022), while triangle points denote clusters new to this DR19 analysis. The solid green lines (RGC = 5, 8, 10, 12, 14 kpc) delineate the annuli used for analyzing azimuthal gradients (see Section 5.3 and Figure 10). The pink dashed lines indicate the boundaries of the azimuthal slices used for analyzing radial gradients (see Section 5.3 and Figure 9). The gray dashed line shows the solar Galactocentric radius used in this work (R = 8.34 kpc).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse