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From One to Two: A Second Binary Millisecond Pulsar in the Globular Cluster M92 (NGC 6341)

  • Authors: Dejiang Yin, Li-yun Zhang, Baoda Li, Yinfeng Dai, Lin Wang, Qiuyu Yu, Yujie Lian

Dejiang Yin et al 2026 The Astrophysical Journal Letters 1004 .

  • Provider: AAS Journals

Caption: Figure 4.

Acceleration model for M92. Black curves show the maximum and minimum LOS accelerations (a,GC) predicted by the cluster potential as a function of projected offset (θ). Downward triangles denote independent limits on pulsar accelerations (﹩{a}_{\ell ,P,{\rm{\max }}}﹩), and the vertical dashed line shows the core radius of M92 (﹩{r}_{{\rm{c}}}=0\mathop{.}\limits^{{\rm{^{\prime} }}}26﹩). The value of M92A is from Y. Lian et al. (2025).

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