Radiation-pressure mixing of large dust grains in protoplanetary disks

Nature

Volumn 459, Issue 7244, 2009, Pages 227-229

  Vinkovi, Dejan ^a  

^a UNIVERSITY OF SPLIT   (Croatia)

Author keywords

[No Author keywords available]

Indexed keywords

ASTRONOMY; COMET; CONDENSATION; DUST; EXTRATERRESTRIAL MATTER; GRAIN SIZE; HIGH TEMPERATURE; INFRARED RADIATION; METEORITE;

ARTICLE; CRYSTAL; DENSITY; GEOMETRY; GRAIN DUST; GRAVITY; INFRARED RADIATION; INTERFEROMETER; LUMINANCE; MOLECULAR INTERACTION; MOLECULAR SIZE; OPTICAL DEPTH; PRESSURE; PRIORITY JOURNAL; RADIATION ABSORPTION; RADIATION PROCESSING; RADIATION SCATTERING; SOLID; TEMPERATURE;

EID: 66149094140     PISSN: 00280836     EISSN: 14764687     Source Type: Journal    
DOI: 10.1038/nature08032     Document Type: Article

References (30)

1. Brownlee, D. et al. Comet 81P/Wild 2 under a microscope. Science 314, 1711-1716 (2006).
2. Wooden, D. H., Harker, D. E. & Brearley, A. J. in Chondrites and the Protoplanetary Disk (eds Krot, A. N., Scott, E. R. D. & Reipurth, B.) 774-808 (ASP Conference Series Vol. 341, 2005).
3. van Boekel, R. et al. The building blocks of planets within the 'terrestrial' region of protoplanetary disks. Nature 432, 479-482 (2004).
4. Hill, H. G. M., Grady, C. A., Nuth, J. A. III, Hallenbeck, S. L. & Sitko, M. L. Constraints on nebular dynamics and chemistry based on observations of annealed magnesium silicate grains in comets and in disks surrounding Herbig Ae/Be stars. Proc. Natl Acad. Sci. USA 98, 2182-2187 (2001).
5. Shu, F. H., Shang, H. & Lee, T. Toward an astrophysical theory of chondrites. Science 271, 1545-1552 (1996).
6. Ciesla, F. J. Outward transport of high-temperature materials around the midplane of the solar nebula. Science 318, 613-615 (2007).
7. Boss, A. P. Mixing in the solar nebula: Implications for isotopic heterogeneity and large-scale transport of refractory grains. Earth Planet. Sci. Lett. 268, 102-109 (2008).
8. Klahr, H., Różyczka, M., Dziourkevitch, N., Wünsch, R. & Johansen, A. in Planet Formation (eds Klahr, H. & Brandner, W.) 42-63 (Cambridge Univ. Press, 2006).
9. Hubickyj, O. in Planet Formation (eds Klahr, H. & Brandner, W.) 163-178 (Cambridge Univ. Press, 2006).
10. Matsumura, S. & Pudritz, R. E. Dead zones and extrasolar planetary properties. Mon. Not. R. Astron. Soc. 365, 572-584 (2006).
11. Shang, H., Li, Z.-Y. & Hirano, N. in Protostars and Planets V (eds Reipurth, B., Jewitt, D. & Keil, K.) 261-276 (Univ. Arizona Press, 2007).
12. Boss, A. P. Evolution of the solar nebula. VII. Formation and survival of protoplanets formed by disk instability. Astrophys. J. 629, 535-548 (2005).
13. Takeuchi, T. & Lin, D. N. C. Surface outflow in optically thick dust disks by radiation pressure. Astrophys. J. 593, 524-533 (2003).
14. Vinkovic, D. Temperature inversion on the surface of externally heated optically thick multigrain dust clouds. Astrophys. J. 651, 906-913 (2006).
15. Millan-Gabet, R. et al. in Protostars and Planets V (eds Reipurth, B., Jewitt, D. & Keil, K.) 539-554 (Univ. Arizona Press, 2007).
16. Vinković, D. & Jurkić, T. Relation between the luminosity of young stellar objects and their circumstellar environment. Astrophys. J. 658, 462-479 (2007).
17. Isella, A. & Natta, A. The shape of the inner rim in proto-planetary disks. Astron. Astrophys. 438, 899-907 (2005).
18. Alexander, R. From discs to planetesimals: Evolution of gas and dust discs. N. Astron. Rev. 52, 60-77 (2008).
19. Chiang, E. I. & Goldreich, P. Spectral energy distributions of T Tauri stars with passive circumstellar disks. Astrophys. J. 490, 368-376 (1997).
20. Fujiwara, D. & Watanabe, S. Protostars and Planets V, Proceedings of the Conference 8237 (Lunar and Planetary Institute, 2005).
21. Voshchinnikov, N. V. & Henning, T. Is the silicate emission feature only influenced by grain size? Astron. Astrophys. 483, L9-L12 (2008).
22. Pinte, C. et al. Probing dust grain evolution in IM Lupi's circumstellar disc. Multi-wavelength observations and modelling of the dust disc. Astron. Astrophys. 489, 633-650 (2008).
23. Jones, R. H., Lee, T., Connolly, H. C. Jr, Love, S. G. & Shang, H. in Protostars and Planets IV (eds Mannings, V., Boss, A. P. & Russell, S. S.) 927-962 (Univ. Arizona Press, 2000).
24. Wuchterl, G. & Tscharnuter, W. M. From clouds to stars. Protostellar collapse and the evolution to the pre-main sequence I. Equations and evolution in the Hertzsprung-Russell diagram. Astron. Astrophys. 398, 1081-1090 (2003).
25. van Boekel, R. et al. A 10 μm spectroscopic survey of Herbig Ae star disks: Grain growth and crystallization. Astron. Astrophys. 437, 189-208 (2005).
26. Sargent, B. et al. Dust processing in disks around T Tauri stars. Astrophys. J. 645, 395-415 (2006).
27. Watson, D. M. et al. Crystalline silicates and dust processing in the protoplanetary disks of the Taurus young cluster. Astrophys. J. Suppl. Ser. 180, 84-101 (2009).
28. Schegerer, A. A., Wolf, S., Ratzka, Th. & Leinert, Ch. The T Tauri star RY Tauri as a case study of the inner regions of circumstellar dust disks. Astron. Astrophys. 478, 779-793 (2008).
29. Dorschner, J., Begemann, B., Henning, T., Jaeger, C. & Mutschke, H. Steps toward interstellar silicate mineralogy. II. Study of Mg-Fe-silicate glasses of variable composition. Astron. Astrophys. 300, 503-520 (1995).
30. Jaeger, C. et al. Steps toward interstellar silicate mineralogy. IV. The crystalline revolution. Astron. Astrophys. 339, 904-916 (1998).