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Pebble Delivery for Inside-Out Planet Formation

Published online by Cambridge University Press:  05 January 2015

Xiao Hu ,
Jonathan C. Tan  and
Sourav Chatterjee
Xiao Hu
Affiliation:
Department of Astronomy, University of Florida, 32611, Gainesville, Florida, USA. email: [email protected], [email protected]
Jonathan C. Tan
Affiliation:
Department of Astronomy, University of Florida, 32611, Gainesville, Florida, USA. email: [email protected], [email protected]
Sourav Chatterjee
Affiliation:
Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Department of Physics & Astronomy, Northwestern University, Evanston, IL 60208, USA. email: [email protected]
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Abstract

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Inside-Out Planet Formation (IOPF; Chatterjee & Tan 2014, hereafter CT14) is a scenario for sequential in situ planet formation at the pressure traps of retreating dead zone inner boundaries (DZIBs) motivated to explain the many systems with tightly packed inner planets (STIPs) discovered by Kepler. The scenario involves build-up of a pebble-dominated protoplanetary ring, supplied by radial drift of pebbles from the outer disk. It may also involve further build-up of planetary masses to gap-opening scales via continued pebble accretion. Here we study radial drift & growth of pebbles delivered to the DZIB in fiducial IOPF disk models.

Keywords

planetary systems: protoplanetary disksplanetary systems: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S310: Complex Planetary Systems , July 2014 , pp. 66 - 69
Copyright
Copyright © International Astronomical Union 2014 

References

Armitage, P. J. 2010, Astrophysics of Planet Formation, Cambridge University Press, 2010Google Scholar
Birnstiel, T., Klahr, H., & Ercolano, B. 2012, A&A, 539, 148Google Scholar
Chatterjee, S. & Tan, J. C. 2014, ApJ, 780, 53CrossRefGoogle Scholar
Chiang, E. & Laughlin, G. 2013, MNRAS, 431, 3444CrossRefGoogle Scholar
Guillot, T, Ida, S. & Ormel, C. W. 2014, arXiv: 1409.7328Google Scholar
Hands, T. O., Alexander, R. D., & Dehnen, W. 2014, arXiv: 1409.0532Google Scholar
Hansen, B. M. S. & Murray, N. 2012, ApJ, 751, 158CrossRefGoogle Scholar
Hansen, B. M. S. & Murray, N. 2013, ApJ, 775, 53CrossRefGoogle Scholar
Zhu, Z., Stone, J. M., & Rafikov, R. R. 2013 ApJ, 768, 143CrossRefGoogle Scholar