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Advances in Astronomy
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2012
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Article
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Fig 7
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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.