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UOCS XIV: Study of the Open Cluster NGC 2627 Using UVIT/AstroSat

  • Authors: Pinapati Saketh, Anju Panthi, Kaushar Vaidya

Pinapati Saketh et al 2024 The Astronomical Journal 168 .

  • Provider: AAS Journals

Caption: Figure 3.

The radial density profile of the cluster members with membership probabilities greater than 0.8, with the error bars representing 1σ Poisson errors. In the bottom left corner, the parameters (normalization factor, core radius, and tidal radius) obtained from the fit with King’s function are shown.

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