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Testing properties of the Galactic center black hole using stellar orbits

PHYSICAL REVIEW D, no. 6 (2010)

Cited: 130|Views25

Abstract

The spin and quadrupole moment of the supermassive black hole at the Galactic center can in principle be measured via astrometric monitoring of stars orbiting at milliparsec distances, allowing tests of general relativistic "no-hair" theorems [23]. One complicating factor is the presence of perturbations from other stars, which may induce...More

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