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Probing the Spacetime around Sagittarius A* with Radio Pulsars

  • Pfahl E
  • Loeb A
The Astrophysical Journal (2004) 615(1) 253-258
DOI: 10.1086/423975
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Abstract

The supermassive black hole at the Galactic center harbors a bound cluster of massive stars that should leave neutron-star remnants. Extrapolating from the available data, we estimate that 100-1000 radio pulsars may presently orbit Sgr A* with periods of

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APA

Pfahl, E., & Loeb, A. (2004). Probing the Spacetime around Sagittarius A* with Radio Pulsars. The Astrophysical Journal, 615(1), 253–258. https://doi.org/10.1086/423975

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