Observational signatures of the black hole Mass Distribution in the Galactic Center

24 Feb 2020 Emami Razieh Center for Astrophysics, Harvard-Smithsonian Loeb Abraham Center for Astrophysics, Harvard-Smithsonian

We simulate the star cluster, made of stars in the main sequence and different black hole (BH) remnants, around SgrA* at the center of the Milky Way galaxy. Tracking stellar evolution, we find the BH remnant masses and construct the BH mass function... (read more)

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Categories


  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • ASTROPHYSICS OF GALAXIES