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The dust environment of comet 67P/Churyumov-Gerasimenko from Rosetta OSIRIS and VLT observations in the 4.5 to 2.9 AU heliocentric distance range inbound

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

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Sierks,  H.
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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Agarwal,  J.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Gutierrez-Marques,  P.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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

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Kovacs,  G.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Kramm,  J.-R.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Oklay,  N.
Department Sun and Heliosphere, 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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Vincent,  J. B.
IMPRS on Physical Processes in the Solar System and Beyond, 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

Moreno, F., Snodgrass, C., Hainaut, O., Tubiana, C., Sierks, H., Barbieri, C., et al. (2016). The dust environment of comet 67P/Churyumov-Gerasimenko from Rosetta OSIRIS and VLT observations in the 4.5 to 2.9 AU heliocentric distance range inbound. Astronomy and Astrophysics, 587: A155. doi:10.1051/0004-6361/201527564.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002D-168D-D
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