arXiv · 1404.4259
On the RZ Draconis Sub-stellar Circumbinary Companions Stability Study of the Proposed Sub-stellar Circumbinary System
Abstract
In this work we revisit the proposed multi-circumbinary system RZ Dra. We find the proposed system to be highly unstable. We attempt to find a best-fit light-travel time model rendering the orbits to follow stable orbits. We found a best-fit solution, but the resulting orbits also exhibit short-term orbital instabilities. We therefore conclude that the observed timing variation must be due to other astrophysical effects causing a change in the binary orbital period. Follow-up observations of this system is encouraged.
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Tobias C. Hinse, Jonathan Horner, Jae Woo Lee, Robert A. Wittenmyer, Chung-Uk Lee, Jang-Ho Park Jonathan P. Marshall. 2014-04-16. On the RZ Draconis Sub-stellar Circumbinary Companions Stability Study of the Proposed Sub-stellar Circumbinary System. https://doi.org/10.1051/0004-6361/201423799
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