Stability of planets orbiting BD + 31deg643

Details Stability of planets orbiting BD + 31deg643 Stability of planets orbiting BD + 31deg643

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.291l..47b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 291, p. L47, L48

Astronomy and Astrophysics

Astronomy

1

Extrasolar Planets, Binary Stars, Solar Orbits, Center Of Mass, Stellar Luminosity, Planetary Systems, Digital Simulation, Elliptical Orbits

Scientific paper

We discuss the possibility of the presence of planetary bodies orbiting BD + 31deg643. We show that, beyond 1000 au from the center of mass of the binary system, the presence of planetary embryos in the recently discovered circumbinary disk is possible. We also show that the central depletion observed in the disk structure is a result of the tidal interaction with the binary.

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