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

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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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-002C-F2C7-1 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-002C-F2C8-0

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Creators:
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: Date issued: 2016

Publication Status: Issued

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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: -