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Distribution of water around the nucleus of comet 67P/Churyumov-Gerasimenko at 3.4 AU from the Sun as seen by the MIRO instrument on Rosetta

MPS-Authors
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Rezac,  L.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Jarchow,  C.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Hartogh,  P.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Biver, N., Hofstadter, M., Gulkis, S., Bockeleé-Morvan, D., Choukroun, M., Lellouch, E., et al. (2015). Distribution of water around the nucleus of comet 67P/Churyumov-Gerasimenko at 3.4 AU from the Sun as seen by the MIRO instrument on Rosetta. Astronomy and Astrophysics, 583: A3. doi:10.1051/0004-6361/201526094.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0028-1F1C-C
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