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The HCN molecule as a tracer of the nucleus rotation of comet 73P-C/Schwassmann-Wachmann 3

MPS-Authors
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Drahus,  M.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

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Küppers,  M.
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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Paganini,  L.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
IMPRS on Physical Processes in the Solar System and Beyond, 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

Drahus, M., Küppers, M., Jarchow, C., Paganini, L., Hartogh, P., & Villanueva, G. L. (2010). The HCN molecule as a tracer of the nucleus rotation of comet 73P-C/Schwassmann-Wachmann 3. Astronomy and Astrophysics, 510: A55. doi:10.1051/0004-6361/20078882.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-032F-2
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