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Black Hole Mass and Spin from the 2:3 Twin-peak QPOs in Microquasars

  • Authors: Soumen Mondal

MONDAL 2010 The Astrophysical Journal 708 1442.

  • Provider: AAS Journals

Caption: Figure 4.

Variation of the angular momentum ( l) at inner edge with the extreme shock locations. Comparing the viscous and inviscid accretion flows for a = 0.0 or 0.50, it is obvious that the shocks occur extremum in the case of inviscid flow independent of viscosity parameter, though for higher a, the extreme shock location is more closer.

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