Advances in Astronomy / 2012 / Article / Fig 7

Review Article

Testing the No-Hair Theorem with Sgr A*

Figure 7

Typical timing residuals for a radio pulsar in an orbit around a black hole with a mass of due to the presence of a nonvanishing quadrupole moment [31]. For Sgr A*, such residuals will have a similar shape but with a larger amplitude.
486750.fig.007

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