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Rapidly Spinning Compact Stars with Deconfinement Phase Transition

  • Authors: Tuna Demircik, Christian Ecker, and Matti Järvinen

2021 The Astrophysical Journal Letters 907 L37.

  • Provider: AAS Journals

Caption: Figure 3.

Density profile of static (left) and maximally rotating (right) stars with 1.4 M (top) and 2 M (bottom) for the stiff model. The black dashed line is the isocontour at matching density n = 1.6 ns and in white regions n/ns < 10−13.

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