Figure 3 from Pulsar J1411+2551: A Low-mass Double Neutron Star System

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Pulsar J1411+2551: A Low-mass Double Neutron Star System

Authors: J. G. Martinez, K. Stovall, P. C. C. Freire, J. S. Deneva, T. M. Tauris, A. Ridolfi, N. Wex, F. A. Jenet, M. A. McLaughlin, and M. Bagchi

2017 The Astrophysical Journal Letters 851 L29.

Provider: AAS Journals

Caption: Figure 3.

Blue points represent the spin period of the recycled pulsars in DNS systems as a function of their orbital period. PSR J1411+2551 is represented by the red star. The gray line represents Equation (4). For a detailed discussion, see Tauris et al. (2017).

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