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  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. (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.

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Lorek, S.1, 2, Author              
Gundlach, B., Author
Lacerda, P.2, 3, Author              
Blum, J., Author
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2Max Planck Research Group in Cometary Science, Max Planck Institute for Solar System Research, Max Planck Society, ou_2265635              
3Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              

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 MPIS_GROUPS: Research Group Cometary Science
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 Dates: 2016
 Publication Status: Published in print
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 Rev. Type: Peer
 Identifiers: DOI: 10.1051/0004-6361/201526565
BibTex Citekey: Lorek:2016-221
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 587 Sequence Number: A128 Start / End Page: - Identifier: -