By Akyea E.C., Meek D.W. (eds.)
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Gas in the coldest disk regions can be traced through CO rotational lines; such studies also suggest a gas depletion by 10 Myr. The combined astronomical evidence shows that: (1) dust disks dissipate in 3−8 Myr via rapid inside-out dispersal; (2) gas dissipates in a similar, or perhaps even shorter timescale. 18 D. Apai and D. S. Lauretta The Solar System, in comparison, offers two lines of evidence to constrain the timescale for the lifetime of the proto-solar nebula and the epoch of planetesimal formation.
Thus, the crystalline magnesium silicate minerals observed in protoplanetary disks may result from thermal annealing of amorphous magnesium and iron silicate condensates. In contrast, shock annealing produces both crystalline magnesium and iron silicates. In addition, experiments demonstrate that the spectral properties of Planet formation and protoplanetary dust 13 annealing silicate smoke grains are highly dependent on their thermal history. Variations in the mid-infrared spectra occur in stages as crystals grow first on the surface, and then in the inner volume, until they merge into a single crystal.
2000, Astronomy and Astrophysics, 357, 325. van Dishoeck, E. F. 2004, Annual Review of Astronomy and Astrophysics, 42, 119. Walmsley, C. , Flower, D. , & Pineau des Forêts, G. 2004, Astronomy and Astrophysics, 418, 1035. Williams, J. , Andrews, S. , & Wilner, D. J. 2005, Astrophysical Journal, 634, 495. Yin, Q. , & Hutcheon, I. D. 2007, Astrophysical Journal, 662, L43. Wyatt, M. C. 2008, Annual Review of Astronomy and Astrophysics, 46, 339. Zolensky, M. , Zega, T. , et al. 2006, Science, 314, 1735.
Catalytic Aspects of Metal Phosphine Complexes by Akyea E.C., Meek D.W. (eds.)