Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-20T16:21:09.976Z Has data issue: false hasContentIssue false
  • English
  • Français

Circumstellar disk evolution: Constraining theories of planet formation

Published online by Cambridge University Press:  01 October 2008

Michael R. Meyer
Michael R. Meyer*
Affiliation:
Steward Observatory, The University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721 (USA)
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Observations of circumstellar disks around stars as a function of stellar properties such as mass, metallicity, multiplicity, and age, provide constraints on theories concerning the formation and evolution of planetary systems. Utilizing ground- and space-based data from the far–UV to the millimeter, astronomers can assess the amount, composition, and location of circumstellar gas and dust as a function of time. We review primarily results from the Spitzer Space Telescope, with reference to other ground- and space-based observations. Comparing these results with those from exoplanet search techniques, theoretical models, as well as the inferred history of our solar system, helps us to assess whether planetary systems like our own, and the potential for life that they represent, are common or rare in the Milky Way galaxy.

Keywords

solar system: formationstars: circumstellar matterpre–main-sequenceplanetary systems: protoplanetary disksplanetary systems: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S258: The Ages of Stars , October 2008 , pp. 111 - 122
Copyright
Copyright © International Astronomical Union 2009

References

Alexander, R. D. & Armitage, P. J. 2007, MNRAS, 375, 500CrossRefGoogle Scholar
Andrews, S. M. & Williams, J. P. 2005, ApJ, 631, 1134CrossRefGoogle Scholar
Apai, D., et al. 2008, ApJ, 672, 1196CrossRefGoogle Scholar
Ardila, D. R., et al. 2004, ApJ, 617, L147CrossRefGoogle Scholar
Bergin, E., Aikawa, Y., Blake, G., & van Dishoeck, E. 2007, Protostars & Planets V, 751Google Scholar
Bitner, M. A., et al. 2008, ApJ, 688, 1326CrossRefGoogle Scholar
Bouwman, J., et al. 2008, ApJ, 683, 479CrossRefGoogle Scholar
Bryden, G., et al. 2006, ApJ, 636, 1098CrossRefGoogle Scholar
Canup, R. M. 2004, ARAA, 42, 441CrossRefGoogle Scholar
Carpenter, J. M., Mamajek, E. E., Hillenbrand, L. A., & Meyer, M. R. 2006, ApJ, 651, L49CrossRefGoogle Scholar
Carpenter, J. M., et al. 2008, ApJS, 179, 423CrossRefGoogle Scholar
Carpenter, J. M., et al. 2009, ApJS, 181, 197CrossRefGoogle Scholar
Carr, J. S. & Najita, J. R. 2008, Science, 319, 1504CrossRefGoogle Scholar
Cieza, L., et al. 2007, ApJ, 667, 308CrossRefGoogle Scholar
Cortes, S., et al. 2009, ApJ, in press (arXiv:0903.3801).Google Scholar
Cumming, A., Butler, R. P., Marcy, G. W., Vogt, S. S., Wright, J. T., & Fischer, D. A. 2008, PASP, 120, 531CrossRefGoogle Scholar
Currie, T., Kenyon, S. J., Balog, Z., Rieke, G., Bragg, A., & Bromley, B. 2008, ApJ, 672, 558CrossRefGoogle Scholar
Dent, W. R. F., Greaves, J. S., & Coulson, I. M. 2005, MNRAS, 359, 663CrossRefGoogle Scholar
Durisen, R. H., Boss, A. P., Mayer, L., Nelson, A. F., Quinn, T., & Rice, W. K. M. 2007, Protostars and Planets V, 607Google Scholar
Dutrey, A., Guilloteau, S. & Ho, P. 2007, Protostars and Planets V, 495Google Scholar
Ercolano, B., Drake, J. J., Raymond, J. C., & Clarke, C. C. 2008, ApJ, 688, 398CrossRefGoogle Scholar
Espaillat, C., Calvet, N., D'Alessio, P., Hernández, J., Qi, C., Hartmann, L., Furlan, E., & Watson, D. M. 2007, ApJ, 670, L135CrossRefGoogle Scholar
Fischer, D. A. & Valenti, J. 2005, ApJ, 622, 1102CrossRefGoogle Scholar
Gatti, T., Natta, A., Randich, S., Testi, L., & Sacco, G. 2008, A&A, 481, 423Google Scholar
Gautier, T. N. III, et al. 2007, ApJ, 667, 527CrossRefGoogle Scholar
Goldreich, P., Lithwick, Y., & Sari, R. 2004, ARAA, 42, 549CrossRefGoogle Scholar
Gorti, U. & Hollenbach, D. 2004, ApJ, 613, 424CrossRefGoogle Scholar
Gorti, U. & Hollenbach, D. 2009, ApJ, 690, 1539CrossRefGoogle Scholar
Greaves, J. S., Fischer, D. A., & Wyatt, M. C. 2006, MNRAS, 366, 283CrossRefGoogle Scholar
Greaves, J. S., Stauffer, J. R., Collier Cameron, A., Meyer, M. R., & Sheehan, C. K. W. 2009, MNRAS, 394, L36CrossRefGoogle Scholar
Haisch, K. E. Jr., Lada, E. A., & Lada, C. J. 2001, ApJ, 553, L153CrossRefGoogle Scholar
Hartigan, P., Edwards, S., & Ghandour, L. 1995, ApJ, 452, 736CrossRefGoogle Scholar
Hartmann, L. 1998, Accretion processes in star formation/Lee Hartmann. Cambridge, UK; New York: Cambridge University Press, 1998. (Cambridge astrophysics series; 32).Google Scholar
Hartmann, L., Calvet, N., Gullbring, E., & D'Alessio, P. 1998, ApJ, 495, 385CrossRefGoogle Scholar
Hillenbrand, L. A. 2008, Physica Scripta Volume T, 130, 014024CrossRefGoogle Scholar
Hillenbrand, L. A., et al. 2008, ApJ, 677, 630CrossRefGoogle Scholar
Ida, S. & Lin, D. N. C. 2008, ApJ, 673, 487CrossRefGoogle Scholar
Ireland, M. J. & Kraus, A. L. 2008, ApJ, 678, L59CrossRefGoogle Scholar
Jacobsen, S. B. 2005, Geochimica et Cosmochimica Acta Supplement, 69, 386Google Scholar
Johnson, J. A., Butler, R. P., Marcy, G. W., Fischer, D. A., Vogt, S. S., Wright, J. T., & Peek, K. M. G. 2007, ApJ, 670, 833CrossRefGoogle Scholar
Kalas, P., et al. 2008, Science, 322, 1345CrossRefGoogle Scholar
Kenyon, S. J. & Bromley, B. C. 2004, ApJ, 602, L133CrossRefGoogle Scholar
Kenyon, S. J. & Bromley, B. C. 2008, ApJS, 179, 451CrossRefGoogle Scholar
Laskar, J. 1994, A&A, 287, L9Google Scholar
Lissauer, J. J. & Stevenson, D. J. 2007, Protostars and Planets V, 591Google Scholar
Lovis, C., et al. 2006, Nature, 441, 305CrossRefGoogle Scholar
Marois, C., Macintosh, B., Barman, T., Zuckerman, B., Song, I., Patience, J., Lafrenière, D., & Doyon, R. 2008, Science, 322, 1348CrossRefGoogle Scholar
Mayor, M., et al. 2009, A&A, 493, 639Google Scholar
Merín, B., et al. 2008, ApJS, 177, 551CrossRefGoogle Scholar
Meyer, M. R., Calvet, N., & Hillenbrand, L. A. 1997, AJ, 114, 288CrossRefGoogle Scholar
Meyer, M. R., et al. 2006, PASP, 118, 1690CrossRefGoogle Scholar
Meyer, M. R., Backman, D. E., Weinberger, A. J., & Wyatt, M. C. 2007, Protostars and Planets V, 573Google Scholar
Meyer, M. R., et al. 2008, ApJ, 673, L181CrossRefGoogle Scholar
Monin, J.-L., Clarke, C. J., Prato, L., & McCabe, C. 2007, Protostars and Planets V, 395Google Scholar
Moro-Martín, A., et al. 2007a, ApJ, 658, 1312CrossRefGoogle Scholar
Moro-Martín, A., et al. 2007b, ApJ, 668, 1165CrossRefGoogle Scholar
Murison, M. A., Lecar, M., & Franklin, F. A. 1994, AJ, 108, 2323CrossRefGoogle Scholar
Muzerolle, J., Calvet, N., Hartmann, L., & D'Alessio, P. 2003, ApJ, 597, L149CrossRefGoogle Scholar
Nagasawa, M., Thommes, E. W., Kenyon, S. J., Bromley, B. C., & Lin, D. N. C. 2007, Protostars and Planets V, 639Google Scholar
Najita, J. R., Strom, S. E., & Muzerolle, J. 2007, MNRAS, 378, 369CrossRefGoogle Scholar
Pascucci, I., et al. 2006, ApJ, 651, 1177CrossRefGoogle Scholar
Pascucci, I., Apai, D., Hardegree-Ullman, E. E., Kim, J. S., Meyer, M. R., & Bouwman, J. 2008a, ApJ, 673, 477CrossRefGoogle Scholar
Pascucci, I., Apai, D., Luhman, K., Henning, T., Bouwman, J., Meyer, M., Lahuis, F., & Natta, A. 2009, ApJ, in press (arXiv:0810.2552)Google Scholar
Pontoppidan, K. M., Blake, G. A., van Dishoeck, E. F., Smette, A., Ireland, M. J., & Brown, J. 2008, ApJ, 684, 1323CrossRefGoogle Scholar
Roccatagliata, V., Henning, T., Wolf, S., Rodmann, J., Corder, S., Carpenter, J. M., Meyer, M., & Dowell, D. 2009, arXiv:0902.0338Google Scholar
Sanders, I. S. & Taylor, G. J. 2005, Chondrites and the Protoplanetary Disk, 341, 915Google Scholar
Santos, N. C., Israelian, G., & Mayor, M. 2004, A&A, 415, 1153Google Scholar
Scott, E. R. D. 2007, Annual Review of Earth and Planetary Sciences, 35, 577CrossRefGoogle Scholar
Siegler, N., Muzerolle, J., Young, E. T., Rieke, G. H., Mamajek, E. E., Trilling, D. E., Gorlova, N., & Su, K. Y. L. 2007, ApJ, 654, 580CrossRefGoogle Scholar
Shu, F., Najita, J., Ostriker, E., Wilkin, F., Ruden, S., & Lizano, S. 1994, ApJ, 429, 781CrossRefGoogle Scholar
Silverstone, M. D., et al. 2006, ApJ, 639, 1138CrossRefGoogle Scholar
Skrutskie, M. F., Dutkevitch, D., Strom, S. E., Edwards, S., Strom, K. M., & Shure, M. A. 1990, AJ, 99, 1187CrossRefGoogle Scholar
Strom, K. M., Strom, S. E., Edwards, S., Cabrit, S., & Skrutskie, M. F. 1989, AJ, 97, 1451CrossRefGoogle Scholar
Su, K. Y. L., et al. 2006, ApJ, 653, 675CrossRefGoogle Scholar
Trilling, D. E., et al. 2007, ApJ, 658, 1289CrossRefGoogle Scholar
Trilling, D. E., et al. 2008, ApJ, 674, 1086CrossRefGoogle Scholar
Tsiganis, K., Gomes, R., Morbidelli, A., & Levison, H. F. 2005, Nature, 435, 459CrossRefGoogle Scholar
Watson, D. M., et al. 2009, ApJS, 180, 84CrossRefGoogle Scholar
Weidenschilling, S. J. 1977, MNRAS, 180, 57CrossRefGoogle Scholar
Werner, M., Fazio, G., Rieke, G., Roellig, T. L., & Watson, D. M. 2006, ARAA, 44, 269CrossRefGoogle Scholar
Wyatt, M. C., Smith, R., Greaves, J. S., Beichman, C. A., Bryden, G., & Lisse, C. M. 2007, ApJ, 658, 569CrossRefGoogle Scholar
Wyatt, M. C. 2008, ARAA, 46, 339CrossRefGoogle Scholar