Abstract
We present a new analysis of the dynamics of the planetary system around the pulsar B1257 + 12. A semianalytical theory of perturbation between terrestrial-mass planets B and C is developed and applied to improve the multiorbit timing formula for this object. We use numerical simulations of the pulse arrival times for PSR B1257 + 12 to demonstrate that our new timing model can serve as a tool to determine the masses of the two planets. Subject headings: celestial mechanics, stellar dynamics - planetary systems -pulsars: individual (PSR B1257 + 12).
Original language | English (US) |
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Pages (from-to) | 921-926 |
Number of pages | 6 |
Journal | Astrophysical Journal |
Volume | 544 |
Issue number | 2 PART 1 |
DOIs | |
State | Published - Dec 1 2000 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science