A Black Hole in the Galactic Center Complex IRS 13E

@article{Schoedel2005ABH,
  title={A Black Hole in the Galactic Center Complex IRS 13E},
  author={R. Schoedel and A. Eckart and C. Iserlohe and R. Genzel and T. Ott},
  journal={The Astrophysical Journal},
  year={2005},
  volume={625}
}
  • R. Schoedel, A. Eckart, +2 authors T. Ott
  • Published 2005
  • Physics
  • The Astrophysical Journal
  • The IRS 13E complex is an unusual concentration of massive, early-type stars at a projected distance of ~0.13 pc from the Milky Way's central supermassive black hole Sagittarius A* (Sgr A*). Because of their similar proper motion and their common nature as massive, young stars, it has recently been suggested that IRS 13E may be the remnant of a massive stellar cluster containing an intermediate-mass black hole (IMBH) that binds its members gravitationally in the tidal field of Sgr A*. Here, we… CONTINUE READING
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    References

    SHOWING 1-10 OF 25 REFERENCES
    A star in a 15.2-year orbit around the supermassive black hole at the centre of the Milky Way
    • 714
    • PDF
    Young Stars at the Center of the Milky Way
    • 40
    The need for a second black hole at the Galactic center
    • 126
    • PDF
    Stellar Disk in the Galactic Center: A Remnant of a Dense Accretion Disk?
    • 273
    • PDF
    The Stellar Cusp around the Supermassive Black Hole in the Galactic Center
    • 425
    • PDF
    Stellar proper motions in the central 0.1 PC of the galaxy
    • 273
    The Nuclear Cluster of the Milky Way: Star Formation and Velocity Dispersion in the Central 0.5 Parsec
    • 255