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Hydrodynamical simulations of G2 interpreted as a diffuse gas cloud

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

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

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

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Citation

Schartmann, M., Burkert, A., Ballone, A., Alig, C., Gillessen, S., Genzel, R., et al. (2014). Hydrodynamical simulations of G2 interpreted as a diffuse gas cloud. In L. O. Sjouwerman, C. C. Lang, & J. Ott (Eds.), The Galactic Center: Feeding and Feedback in a Normal Galactic Nucleus ( IAU Symposium 303 ) (pp. 324-326). Cambridge, UK: Cambridge University Press.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0019-D870-9
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