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3D AMR simulations of the evolution of the diffuse gas cloud G2 in the Galactic Centre

MPS-Authors
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Schartmann,  M.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Ballone,  A.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Burkert,  A.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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

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

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Eisenhauer,  F.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Plewa,  P. M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Ott,  T.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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George,  E. M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Habibi,  M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Schartmann, M., Ballone, A., Burkert, A., Gillessen, S., Genzel, R., Pfuhl, O., et al. (2017). 3D AMR simulations of the evolution of the diffuse gas cloud G2 in the Galactic Centre. In R. M. Crocker, S. N. Longmore, & G. V. Bicknell (Eds.), The Multi-Messenger Astrophysics of the Galactic Centre (IAU Symposium 322) (pp. 241-242). Cambridge, UK: Cambridge University Press.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002C-C26D-C
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