The old nuclear star cluster in the Milky Way: dynamics, mass, statistical 
parallax, and black hole mass

Chatzopoulos, S.; Fritz, T. K.; Gerhard, O.; Gillessen, S.; Wegg, C.; Genzel, R.; Pfuhl, O.

doi:10.1093/mnras/stu2452

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The old nuclear star cluster in the Milky Way: dynamics, mass, statistical parallax, and black hole mass

MPS-Authors

/persons/resource/persons132055

Chatzopoulos, S.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4692

Gerhard, O.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4768

Gillessen, S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons128242

Wegg, C.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4590

Genzel, R.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4782

Pfuhl, O.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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引用

Chatzopoulos, S., Fritz, T. K., Gerhard, O., Gillessen, S., Wegg, C., Genzel, R., & Pfuhl, O. (2015). The old nuclear star cluster in the Milky Way: dynamics, mass, statistical parallax, and black hole mass. Monthly Notices of the Royal Astronomical Society, 447(1), 948-968. doi:10.1093/mnras/stu2452.

引用: https://hdl.handle.net/11858/00-001M-0000-0026-BE86-4

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