Unveiling the nature of SgrA* with the geodesic motion of S-stars

@article{DellaMonica2022UnveilingTN,
  title={Unveiling the nature of SgrA* with the geodesic motion of S-stars},
  author={Riccardo Della Monica and Ivan de Martino},
  journal={Journal of Cosmology and Astroparticle Physics},
  year={2022},
  volume={2022}
}
Despite the huge improvements guaranteed by future GRAVITY observations of the S0-2 star, these will not be able to unveil the fundamental nature, whether black hole or wormhole, of the central supermassive object. Nevertheless, observing stars orbiting closer to the central gravitational source could allow to distinguish between the black hole and wormhole nature of this object at more than 5σ. Firstly, we have used publicly available astrometric and spectroscopic measurements of the S0-2 star… 
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