# Dynamical properties of binary stars hosting planets in the Galactic   Center

**Authors:** Nazanin Davari, Roberto Capuzzo-Dolcetta

arXiv: 1906.03738 · 2019-06-11

## TL;DR

This paper investigates the dynamical interactions of binary star systems with planets near the Galactic Center's supermassive black hole, focusing on their close encounters and potential effects.

## Contribution

It provides initial insights into the dynamical behavior of binary star-planet systems during close encounters with Sgr A* in the Galactic Center.

## Key findings

- Preliminary analysis of binary star encounters with Sgr A*
- Insights into potential orbital disruptions of planets
- Foundation for future detailed simulations

## Abstract

We present some preliminary results of our work about the close encounter of binary stars hosting planets on S-type orbits with the Sgr A* supermassive black hole in the center of our Galaxy.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1906.03738/full.md

## References

19 references — full list in the complete paper: https://tomesphere.com/paper/1906.03738/full.md

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Source: https://tomesphere.com/paper/1906.03738