Stability of prograde and retrograde planets in circular binary systems

ISSN： 0035-8711

Source： Monthly Notices of the Royal Astronomical Society, Vol.424, Iss.1, 2012-07, pp. : 52-64

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Eccentricities of Planets in Binary Systems

By Takeda Genya Rasio Frederic

Astrophysics and Space Science, Vol. 304, Iss. 1-4, 2006-08 ,pp. : 239-242

Springer Publishing Company

Access to resources Recommend Favorite

Orbital stability of systems of closely-spaced planets, II: configurations with coorbital planets

By Smith Andrew Lissauer Jack

Celestial Mechanics and Dynamical Astronomy, Vol. 107, Iss. 4, 2010-08 ,pp. : 487-500

Springer Publishing Company

Access to resources Recommend Favorite

Regions of dynamical stability for discs and planets in binary stars of the solar neighbourhood

By Jaime Luisa G. Pichardo Barbara Aguilar Luis

Monthly Notices of the Royal Astronomical Society, Vol. 427, Iss. 4, 2012-12 ,pp. : 2723-2733

Oxford University Press

Access to resources Recommend Favorite

On the stability of possible Trojan planets in the habitable zone: an application to the systems HD 147513 and HD 210277

By Funk B. Schwarz R. Süli Á. Érdi B.

Monthly Notices of the Royal Astronomical Society, Vol. 423, Iss. 4, 2012-07 ,pp. : 3074-3082

Oxford University Press

Access to resources Recommend Favorite

Gravitomagnetism: a novel explanation of the precession of planets and binary pulsars

By Arbab Arbab

Astrophysics and Space Science, Vol. 330, Iss. 1, 2010-11 ,pp. : 61-68

Springer Publishing Company

Access to resources Recommend Favorite