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How Do Disks and Planetary Systems in High-mass Open Clusters Differ from Those around Field Stars?

Vincke, K., & Pfalzner, S. (2018). How Do Disks and Planetary Systems in High-mass Open Clusters Differ from Those around Field Stars? Astrophysical Journal, 868: 1, pp. 1. doi:10.3847/1538-4357/aae7d1.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0004-3CF2-8 Version Permalink: https://hdl.handle.net/21.11116/0000-0004-3CF3-7

Genre: Journal Article

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Vincke, K.¹, Author
Pfalzner, S.¹, Author

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1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652

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Free keywords: open clusters and associations: general, planets and satellites: dynamical evolution and stability, protoplanetary disks

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Dates: Date issued: 2018-11

Publication Status: Issued

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Identifiers: DOI: 10.3847/1538-4357/aae7d1
BibTex Citekey: 2018apj...868....1v

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Title: Astrophysical Journal

Source Genre: Journal

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Pages: - Volume / Issue: 868 Sequence Number: 1 Start / End Page: 1 Identifier: -