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Evolution of solids in planet forming disks: The interplay of experiments, simulations, and observations

Published online by Cambridge University Press:  12 October 2020

T. Birnstiel Open the ORCID record for T. Birnstiel [Opens in a new window]
T. Birnstiel*
Affiliation:
University Observatory, Faculty of Physics, Ludwig-Maximilians-Universität München, Scheinerstr. 1, 81679 Munich, Germany email: til.birnstiel@lmu.de
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Abstract

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Circumstellar dust analogues can be studied experimentally to determine their collisional behavior and their optical properties. These results affect simulations of circumstellar disks in various, substantial ways: Collision results determine how dust aggregates grow and how their aerodynamic properties change with time. This determines how solids move throughout the disk, how they accumulate, and how planetesimals might be formed. The optical properties determine the observational signature of these effects and allow us to constrain the spatial distribution of dust in disks, the sizes of the aggregates, as well as the temperature and optical depth of the dust emission. In this contribution, it is discussed how theoretical models and their predictions depend on laboratory results and what we learned about disks from high spatial resolution radio interferometry.

Keywords

planetary systems: protoplanetary diskscircumstellar matterscatteringsubmillimeter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S350: Laboratory Astrophysics: From Observations to Interpretation , April 2019 , pp. 200 - 204
Copyright
© International Astronomical Union 2020

References

Andrews, S. M., Huang, J., Pérez, L. M., et al. 2018, ApJL, 869, L41 CrossRefGoogle Scholar
Avenhaus, H., Quanz, S. P., Garufi, A., et al. 2018, ApJ, 863, 44 CrossRefGoogle Scholar
Banzatti, A., Pinilla, P., Ricci, L., et al. 2015, ApJL, 815, L15 CrossRefGoogle Scholar
Bentez-Llambay, P., & Masset, F. S. 2016, ApJS, 223, 11 CrossRefGoogle Scholar
Birnstiel, T., Dullemond, C. P., & Brauer, F. 2010, A&A, 513, A79 Google Scholar
Birnstiel, T., Klahr, H., & Ercolano, B. 2012, A&A, 539, A148 Google Scholar
Birnstiel, T., Dullemond, C. P., Zhu, Z., et al. 2018, ApJL, 869, L45 CrossRefGoogle Scholar
Blum, J., & Wurm, G. 2008, ARA&A, 46, 21 CrossRefGoogle Scholar
Boudet, N., Mutschke, H., Nayral, C., et al. 2005, ApJ, 633, 272 CrossRefGoogle Scholar
Brauer, F., Dullemond, C. P., & Henning, T. 2008a, A&A, 480, 859 Google Scholar
Brauer, F., Henning, T., & Dullemond, C. P. 2008b, A&A, 487, L1 Google Scholar
Cieza, L. A., Casassus, S., Tobin, J., et al. 2016, Nature, 535, 258 CrossRefGoogle Scholar
Coupeaud, A., Demyk, K., Meny, C., et al. 2011, A&A, 535, 124 Google Scholar
Cridland, A. J., Pudritz, R. E., Birnstiel, T., Cleeves, L. I., & Bergin, E. A. 2017, MNRAS, 469, 3910 CrossRefGoogle Scholar
Cuzzi, J. N., Estrada, P. R., & Davis, S. S. 2014, ApJS, 210, 21 CrossRefGoogle Scholar
Demyk, K., Meny, C., Lu, X. H., et al. 2017a, A&A, 600, A123 Google Scholar
Demyk, K., Meny, C., Leroux, H., et al. 2017b, A&A, 606, A50 Google Scholar
Drrażkowska, J., Alibert, Y., & Moore, B. 2016, A&A, 594, A105 Google Scholar
Drażkowska, J., & Dullemond, C. P. 2014, A&A, 572, A78 Google Scholar
Güttler, C., Blum, J., Zsom, A., Ormel, C. W., & Dullemond, C. P. 2010, A&A, 513, 56 Google Scholar
Huang, J., Andrews, S. M., Dullemond, C. P., et al. 2018a, ApJL, 869, L42 CrossRefGoogle Scholar
Huang, J., Andrews, S. M., Pérez, L. M., et al. 2018b, ApJL, 869, L43 CrossRefGoogle Scholar
Kataoka, A., Okuzumi, S., Tanaka, H., & Nomura, H. 2014, A&A, 568, A42 Google Scholar
Kretke, K. A., & Lin, D. N. C. 2007, ApJL, 664, L55 CrossRefGoogle Scholar
Morbidelli, A., Chambers, J., Lunine, J. I., et al. 2000, Meteorit. Planet. Sci., 35, 1309 CrossRefGoogle Scholar
Nakagawa, Y., Sekiya, M., & Hayashi, C. 1986, Icarus, 67, 375 CrossRefGoogle Scholar
Pinte, C., Dent, W. R. F., Ménard, F., et al. 2016, ApJ, 816, 25 CrossRefGoogle Scholar
Schoonenberg, D., & Ormel, C. W. 2017, A&A, 602, A21 Google Scholar
Tazaki, R., & Tanaka, H. 2018, ApJ, 860, 79 CrossRefGoogle Scholar
Tazaki, R., Tanaka, H., Okuzumi, S., Kataoka, A., & Nomura, H. 2016, ApJ, 823, 70 CrossRefGoogle Scholar
Testi, L., Birnstiel, T., Ricci, L., et al. 2014, PPVI, 339Google Scholar
Whipple, F. L. 1972, From Plasma to Planet, 211Google Scholar