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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 4.

The cumulative radial distributions of equal-mass binary, massive single, and low-mass single populations. The BSSs are within a radius of 10r c , shown by the brown dashed line. The x-axis represents the radial distance in units of the core radius, r c , and the y-axis represents the normalized numbers of the three populations.

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