Masses and Orbital Inclinations of Planets in the PSR B1257+12 System

@article{Konacki2003MassesAO,
  title={Masses and Orbital Inclinations of Planets in the PSR B1257+12 System},
  author={Maciej Konacki and Alex Wolszczan},
  journal={The Astrophysical Journal Letters},
  year={2003},
  volume={591},
  pages={L147 - L150}
}
We present measurements of the true masses and orbital inclinations of the two Earth-mass planets in the PSR B1257+12 system, based on the analysis of their mutual gravitational perturbations detectable as microsecond variations of the arrival times of radio pulses from the pulsar. The 6.2 ms pulsar, PSR B1257+12, has been regularly timed with the Arecibo telescope since late 1990. Assuming the standard pulsar mass of 1.4 M☉, the derived masses of planets B and C are 4.3 ± 0.2 and 3.9 ± 0.2 M… 

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