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A Planetary Nebula from a 5.7 M Progenitor in a 90 Myr M31 Star Cluster

  • Authors: Pinjian Chen, Bingqiu Chen, Xiaodian Chen, Shu Wang, Haibo Yuan

Pinjian Chen et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 1.

Color composite image of the young open cluster AP 210, constructed from archival HST/ACS observations in F475W (blue), F625W+F658N (green), and F814W (red). The PN appears as a bright blue–green point source near the cluster center because of its strong [O III], Hα, and [N II] emission. The white circle indicates the ﹩1\mathop{.}\limits{^{\prime\prime} }5﹩ on-sky diameter of a single Hectospec fiber.

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