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Planet formation in evolving protoplanetary discs

Published online by Cambridge University Press:  06 January 2014

Richard Alexander
Richard Alexander*
Affiliation:
Department of Physics & Astronomy, University of Leicester, Leicester, LE1 7RH, UK email: richard.alexander@leicester.ac.uk
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Abstract

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I attempt to summarize our knowledge of planet formation in evolving protoplanetary discs. I first review the physics of disc evolution and dispersal. For most of the disc lifetime evolution is driven by accretion and photoevaporation, and I discuss how the interplay between these processes shapes protoplanetary discs. I also discuss the observations that we use to test these models, and the major uncertainties that remain. I will then move on to consider planet formation and migration in evolving discs, and discuss how observations of both discs and planets can be used to inform our understanding of protoplanetary disc evolution.

Keywords

protoplanetary discsplanet–disc interactionsplanetary systems

References

Adams, F. C., Hollenbach, D., Laughlin, G., & Gorti, U. 2004, ApJ, 611, 360CrossRefGoogle Scholar
Alexander, R. 2008a, New Astron. Revs., 52, 60CrossRefGoogle Scholar
Alexander, R. D. 2008b, MNRAS 391, L64CrossRefGoogle Scholar
Alexander, R. D. & Armitage, P. J. 2009, ApJ, 704, 989CrossRefGoogle Scholar
Alexander, R. D., Clarke, C. J., & Pringle, J. E. 2006a, MNRAS, 369, 216CrossRefGoogle Scholar
Alexander, R. D., Clarke, C. J., & Pringle, J. E. 2006b, MNRAS, 369, 229Google Scholar
Alexander, R. D. & Pascucci, I. 2012, MNRAS, 422, L82Google Scholar
Alexander, R., Pascucci, I., Andrews, S., Armitage, P., & Cieza, L. 2014, Protostars & Planets VI, in press, arXiv:1311.1819Google Scholar
Andrews, S. M. & Williams, J. P. 2005, ApJ, 631, 1134Google Scholar
Andrews, S. M., Wilner, D. J., Hughes, A. M., Qi, C., & Dullemond, C. P. 2009, ApJ, 700, 1502Google Scholar
Armitage, P. J. 2011, ARAA, 49, 195CrossRefGoogle Scholar
Armitage, P. J., Livio, M., Lubow, S. H., & Pringle, J. E. 2002, MNRAS, 334, 248CrossRefGoogle Scholar
Bae, J., Hartmann, L., Zhu, Z., & Gammie, C. 2013, ApJ, 774, 57CrossRefGoogle Scholar
Bai, X.-N. 2011, ApJ, 739, 50Google Scholar
Bai, X.-N. & Stone, J. M. 2013, ApJ, 769, 76Google Scholar
Balbus, S. A. 2011, in Physical Processes in Circumstellar Disks around Young Stars, ed. Garcia, P. J. V., 237–282Google Scholar
Balbus, S. A. & Hawley, J. F. 1991, ApJ, 376, 214CrossRefGoogle Scholar
Baldovin-Saavedra, C., Audard, M., Carmona, A., et al. 2012, A&A, 543, A30Google Scholar
Beckwith, K., Armitage, P. J., & Simon, J. B. 2011, MNRAS, 416, 361Google Scholar
Bell, C. P. M., Naylor, T., Mayne, N. J., Jeffries, R. D., & Littlefair, S. P. 2013, MNRAS, 434, 806Google Scholar
Calvet, N. & Gullbring, E. 1998, ApJ, 509, 802CrossRefGoogle Scholar
Cieza, L. A., Swift, J. J., Mathews, G. S., & Williams, J. P. 2008, ApJL, 686, L115Google Scholar
Clarke, C. 2011, in Physical Processes in Circumstellar Disks around Young Stars, ed. P. J. V. Garcia, 355–418Google Scholar
Clarke, C. J., Gendrin, A., & Sotomayor, M. 2001, MNRAS, 328, 485CrossRefGoogle Scholar
Ercolano, B. & Owen, J. E. 2010, MNRAS, 406, 1553Google Scholar
Fedele, D., van den Ancker, M. E., Henning, T., Jayawardhana, R., & Oliveira, J. M. 2010, A&A, 510, A72Google Scholar
Feigelson, E., Townsley, L., Güdel, M., & Stassun, K. 2007, Protostars and Planets V, 313Google Scholar
Font, A. S., McCarthy, I. G., Johnstone, D., & Ballantyne, D. R. 2004, ApJ, 607, 890Google Scholar
Fromang, S., Latter, H., Lesur, G., & Ogilvie, G. I. 2013, A&A, 552, A71Google Scholar
Gammie, C. F. 1996, ApJ, 457, 355CrossRefGoogle Scholar
Goldreich, P. & Tremaine, S. 1979, ApJ, 233, 857Google Scholar
Goldreich, P. & Tremaine, S. 1980, ApJ, 241, 425CrossRefGoogle Scholar
Gorti, U., Dullemond, C. P., & Hollenbach, D. 2009, ApJ, 705, 1237Google Scholar
Gorti, U. & Hollenbach, D. 2008, ApJ, 683, 287Google Scholar
Gorti, U. & Hollenbach, D. 2009, ApJ, 690, 1539CrossRefGoogle Scholar
Guillot, T. & Hueso, R. 2006, MNRAS, 367, L47Google Scholar
Gullbring, E., Hartmann, L., Briceno, C., & Calvet, N. 1998, ApJ, 492, 323Google Scholar
Haisch, K. E. Jr., Lada, E. A., & Lada, C. J. 2001, ApJL, 553, L153Google Scholar
Hartmann, L., Calvet, N., Gullbring, E., & D'Alessio, P. 1998, ApJ, 495, 385Google Scholar
Hasegawa, Y. & Pudritz, R. E. 2012, ApJ, 760, 117CrossRefGoogle Scholar
Hillenbrand, L. A. 2009, in IAU Symposium, Vol. 258, ed. Mamajek, E. E., Soderblom, D. R., & Wyse, R. F. G., 81–94Google Scholar
Hollenbach, D., Johnstone, D., Lizano, S., & Shu, F. 1994, ApJ, 428, 654CrossRefGoogle Scholar
Hollenbach, D. & Gorti, U. 2009, ApJ, 703, 1203CrossRefGoogle Scholar
Ida, S. & Lin, D. N. C. 2004, ApJ, 604, 388Google Scholar
Ingleby, L., Calvet, N., Hernández, J., et al. 2011, AJ, 141, 127CrossRefGoogle Scholar
Johnstone, D., Hollenbach, D., & Bally, J. 1998, ApJ, 499, 758CrossRefGoogle Scholar
Jones, M. G., Pringle, J. E., & Alexander, R. D. 2012, MNRAS, 419, 925CrossRefGoogle Scholar
Kley, W. & Nelson, R. P. 2012, ARAA, 50, 211Google Scholar
Koepferl, C. M., Ercolano, B., Dale, J., et al. 2013, MNRAS, 428, 3327Google Scholar
Königl, A. & Salmeron, R. 2011, in Physical Processes in Circumstellar Disks around Young Stars, ed. Garcia, P. J. V., 283–352Google Scholar
Liffman, K. 2003, PASA, 20, 337CrossRefGoogle Scholar
Lodato, G. 2007, Nuovo Cimento Rivista Serie, 30, 293Google Scholar
Lynden-Bell, D. & Pringle, J. E. 1974, MNRAS, 168, 603CrossRefGoogle Scholar
Mamajek, E. E. 2009, in American Institute of Physics Conference Series, ed. Usuda, T., Tamura, M., & Ishii, M., Vol. 1158, 3–10Google Scholar
Mordasini, C., Alibert, Y., & Benz, W. 2009, A&A, 501, 1139Google Scholar
Owen, J. E., Clarke, C. J., & Ercolano, B. 2012, MNRAS, 422, 1880Google Scholar
Owen, J. E., Ercolano, B., & Clarke, C. J. 2011, MNRAS, 412, 13Google Scholar
Owen, J. E., Ercolano, B., Clarke, C. J., & Alexander, R. D. 2010, MNRAS, 401, 1415CrossRefGoogle Scholar
Paardekooper, S.-J. & Papaloizou, J. C. B. 2009, MNRAS, 394, 2283CrossRefGoogle Scholar
Pascucci, I., Gorti, U., & Hollenbach, D. 2012, ApJL, 751, L42CrossRefGoogle Scholar
Pascucci, I. & Sterzik, M. 2009, ApJ, 702, 724Google Scholar
Pascucci, I., Gorti, U., Hollenbach, D., et al. 2006, ApJ, 651, 1177Google Scholar
Pascucci, I., Sterzik, M., Alexander, R. D., et al. 2011, ApJ, 736, 13Google Scholar
Rigliaco, E., Pascucci, I., Gorti, U., Edwards, S., & Hollenbach, D. 2013, ApJ, 772, 60Google Scholar
Sacco, G. G., Flaccomio, E., Pascucci, I., et al. 2012, ApJ, 747, 142Google Scholar
Sargent, A. I. & Beckwith, S. 1987, ApJ, 323, 294Google Scholar
Shu, F. H., Johnstone, D., & Hollenbach, D. 1993, Icarus, 106, 92CrossRefGoogle Scholar
Simon, M. & Prato, L. 1995, ApJ, 450, 824Google Scholar
Throop, H. B. & Bally, J. 2005, ApJL, 623, L149Google Scholar
Wright, J. T., Fakhouri, O., Marcy, G. W., et al. 2011, PASP, 123, 412Google Scholar