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Does the Gamma-Ray Binary LS I + 61°303 Harbor a Magnetar?

  • Authors: Arthur G. Suvorov, Kostas Glampedakis

Arthur G. Suvorov and Kostas Glampedakis 2022 The Astrophysical Journal 940 .

  • Provider: AAS Journals

Caption: Figure 5.

Characteristic strains h 0 from Equation (20) as a function of the poloidal-to-total magnetic energy ratio, Λ, using the dipolar Tolman-VII model (Equation (21)) of Mastrano et al. (2011) for LSI. The colored bands represent the prediction for different B p , with the lower curves having M = 1.4 M and R = 10 km and the upper curves having M = 2 M and R = 14 km. Overlaid are the detection thresholds for aLIGO and ET for a variety of different observation times T obs, as indicated by the labeled dashed lines.

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