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Simulating the Collapse of a Thick Accretion Disk due to a Type I X-Ray Burst from a Neutron Star

  • Authors: P. Chris Fragile, David R. Ballantyne, Thomas J. Maccarone, and Jason W. L. Witry

2018 The Astrophysical Journal Letters 867 L28.

  • Provider: AAS Journals

Caption: Figure 2.

Ratio between the mass accretion rate onto the neutron star for simulations with and without a Type I X-ray burst. The two curves distinguish between burst simulations where Compton cooling is included (red dashed curve) and where it is turned off (green dotted curve). Enhanced accretion of approximately equal magnitude occurs during both simulations, but the effects of Compton cooling boost the accretion rate earlier than PR drag alone.

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