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Gonzalez , Jean-François; Fouchet , Laure; T. Maddison , Sarah; Laibe , Guillaume (2007)
Publisher: HAL CCSD
Languages: English
Types: Conference object
Subjects: planetary systems: protoplanetary disks, [ PHYS.ASTR.CO ] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics, hydrodynamics, methods: numerical, [ SDU.ASTR.CO ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [ SDU.ASTR ] Sciences of the Universe [physics]/Astrophysics [astro-ph]

Classified by OpenAIRE into

arxiv: Astrophysics::Galaxy Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics
6 pages, 5 figures, to appear in the Proceedings of IAU Symp. 249: Exoplanets: Detection, Formation and Dynamics (Suzhou, China); International audience; We investigate the behaviour of dust in protoplanetary disks under the action of gas drag using our 3D, two-fluid (gas+dust) SPH code. We present the evolution of the dust spatial distribution in global simulations of planetless disks as well as of disks containing an already formed planet. The resulting dust structures vary strongly with particle size and planetary gaps are much sharper than in the gas phase, making them easier to detect with ALMA than anticipated. We also find that there is a range of masses where a planet can open a gap in the dust layer whereas it doesn't in the gas disk. Our dust distributions are fed to the radiative transfer code MCFOST to compute synthetic images, in order to derive constraints on the settling and growth of dust grains in observed disks.
  • The results below are discovered through our pilot algorithms. Let us know how we are doing!

    • Barri`ere-Fouchet, L., Gonzalez, J.-F., Murray, J. R., Humble, R. J., & Maddison, S. T. 2005, A&A, 443, 185
    • Dominik, C., Blum, J., Cuzzi, J. N., & Wurm, G. 2007, in: B. Reipurth, D. Jewitt & K. Keil (eds.), Protostars and Planets V (Tucson: University of Arizona Press), p. 783 Dullemond, C. P. & Dominik, C. 2005, A&A, 434, 971
    • Fouchet, L., Maddison, S. T., Gonzalez, J.-F., & Murray, J. R. 2007, A&A, 474, 1037 Garaud, P., Barri`ere-Fouchet, L., & Lin, D. N. C. 2004, ApJ, 603, 292 Johansen, A., Oishi, J. S., Mac Low, M.-M., et al. 2007, Nature, 448, 1022 Laibe, G., Gonzalez, J.-F., Fouchet, L., & Maddison, S.T. 2008, in preparation Maddison, S. T., Fouchet, L., & Gonzalez, J.-F. 2007, Ap&SS, 311, 3 Paardekooper, S.-J. & Mellema, G. 2006, A&A, 453, 1129
    • Pinte, C., M´enard, F., Duchˆene, G., & Bastien, P. 2006, A&A, 459, 797 Pinte, C., Fouchet, L., M´enard, F., Gonzalez, J.-F., & Duchˆene, G. 2007, A&A, 469, 963 Stepinski, T. F. & Valageas, P. 1997, A&A, 319, 1007
    • Varni`ere, P., Bjorkman, J. E., Frank, A., et al. 2006, ApJ, 637, L125 Watson, A. M., Stapelfeldt, K. R., Wood, K., & M´enard, F. 2007, in: B. Reipurth, D. Jewitt & K. Keil (eds.), Protostars and Planets V (Tucson: University of Arizona Press), p. 523 Weidenschilling, S. 1977, MNRAS, 180, 57
    • Wolf, S. & D'Angelo, G. 2005, ApJ, 619, 1114
  • No related research data.
  • No similar publications.
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