Contemporary formation of early Solar System planetesimals at two distinct radial locations
Author:
Funder
Agence Nationale de la Recherche
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-021-01517-7.pdf
Reference50 articles.
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2. Cuzzi, J. N., Hogan, R. C. & Shariff, K. Toward planetesimals: dense chondrule clumps in the protoplanetary nebula. Astrophys. J. 687, 1432–1447 (2008).
3. Simon, J. B., Armitage, P. J., Li, R. & Youdin, A. N. The mass and size distribution of planetesimals formed by the streaming instability. I. The role of self-gravity. Astrophys. J. 822, 55 (2016).
4. Drążkowska, J. & Dullemond, C. P. Can dust coagulation trigger streaming instability? Astron. Astrophys. 572, A78 (2014).
5. Yang, C.-C., Johansen, A. & Carrera, D. Concentrating small particles in protoplanetary disks through the streaming instability. Astron. Astrophys. 606, A80 (2017).
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