Comet formation in collapsing pebble clouds. What cometary bulk density implies 
for the cloud mass and dust-to-ice ratio

Lorek, S.; Gundlach, B.; Lacerda, P.; Blum, J.

doi:10.1051/0004-6361/201526565

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Comet formation in collapsing pebble clouds. What cometary bulk density implies for the cloud mass and dust-to-ice ratio

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Lorek, S.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Max Planck Research Group in Cometary Science, Max Planck Institute for Solar System Research, Max Planck Society;

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Lacerda, P.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
Max Planck Research Group in Cometary Science, Max Planck Institute for Solar System Research, Max Planck Society;

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Lorek, S., Gundlach, B., Lacerda, P., & Blum, J. (2016). Comet formation in collapsing pebble clouds. What cometary bulk density implies for the cloud mass and dust-to-ice ratio. Astronomy and Astrophysics, 587: A128. doi:10.1051/0004-6361/201526565.

Cite as: https://hdl.handle.net/11858/00-001M-0000-002C-F2C7-1

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