Figure 8 from GW190814's Secondary Component with Mass 2.50

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GW190814's Secondary Component with Mass 2.50–2.67 M_⊙ as a Superfast Pulsar

Authors: Nai-Bo Zhang and Bao-An Li

2020 The Astrophysical Journal 902 38.

Provider: AAS Journals

Caption: Figure 8.

Energy density contours on the equatorial (r_e)–polar (r_p) plane with EOS1 (top) and EOS4 (bottom) at the minimum frequency f_2.5 to rotationally support NSs with a mass of M = 2.50 M_⊙.

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