24 Aqr Triple System: New Orbital Solutions and Parameters
Analysis
This paper presents new orbital solutions and fundamental parameters for the 24 Aqr triple star system, utilizing new observations and various analysis techniques. The study is significant because of the system's unique high-eccentricity hierarchical architecture and the recent periastron passage. The derived parameters, including precise masses and a new dynamical parallax, contribute to a better understanding of this complex system. The paper also discusses the possibility of a coplanar orbit and the observational challenges.
Key Takeaways
- •Presents new orbital solutions and fundamental parameters for the 24 Aqr triple star system.
- •Utilizes new speckle interferometry observations from the Lowell Discovery Telescope.
- •Employs various analysis techniques, including ORBITX and Al-Wardat's method.
- •Derives precise masses and a new dynamical parallax.
- •Discusses the possibility of a coplanar orbit.
- •Highlights the need for a large telescope or telescope array for visual resolution of the inner binary.
Reference
“The paper derives precise masses and the complete set of its fundamental parameters for the three components, and introduces a new orbital solution, and a new dynamical parallax.”