Image Details

Choose export citation format:

Time-series Photometric Detection and Physical Characterization of Variable Stars in Four Intermediate- to Old-age Galactic Open Clusters

  • Authors: K. Belwal, D. Bisht, Ing-Guey Jiang, Mohit Singh Bisht, A. Raj, S. K. Chakrabarti, D. Bhowmick

K. Belwal et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 1.

R-band finding charts of the observed fields for the OCs NGC 2192, NGC 2266, NGC 2509, and IC 1369. The images are representative frames from the time-series photometric observations used in this study. Newly identified variable stars are marked with white circles and labeled by their IDs. Yellow plus symbols indicate the cluster centers. The inner red circle denotes the cluster core radius, while the outer blue circle indicates the cluster (limiting) radius, both estimated in the present analysis. The orientation is north up and east to the left, with R.A. and decl. shown in degrees.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse