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26 Apr 2006: 1.0 [24]. The slope of the linethrough data set (h), for silicon carbide particles in a succino-nitrile melt, is! ... Azouni, W. Kalita, M. Yemmou, J. Crystal Growth. 99 (1990) 201.[24] S.

22 Nov 2006: This sensitivity to outliers is a well known feature of the MMI criterion [24]. ... j))}. (24). Each Gaussian component is assumed to be independent of all others.

4 Sep 2006: 1990. 335.87. 80.22. 1990. 5.6. 4.6. 39.9. 24.9. 5.3. 1991. 335.20. ... 81.54. 1991. 5.4. 4.8. 41.7. 24.5. 5.2. 1992. 338.00. 78.85. 4.

19 Apr 2006: Surprisingly, however, the 24 and 70 µm images of Vegaactually have larger radii than the submillimeter ring or mil-limeter clumps (Su et al., 2005). ... Emission (Additional)Vega A0 200 >90 23,24,25 Eridani K2 <1000 60 26,27η Corvi F2 1000 100 28τ

26 Apr 2006: Using equations (3) and (22)–(24), it is possibleto calculate _h, S0 and T0 in terms of far-field properties T1and S1 by eliminating two of the unknowns to obtain aquadratic ... For this simula-tion we used again the values given in Table 1 and Si =

16 Jun 2006: Science (Wash. DC). 208:1454-1457. 24. Ross, M. J., M. W. Klymkowsky, D. ... J. Ultrastruct. R e s 24:454-564. 27. Ziogsheim, H.-P., D.-C. Neugehauer, F.

23 Jul 2006: MP3. 44100 Hz. 123.64 MB. Date: July 24, 2006. Speakers: Revd Michael Roberts.

22 May 2006: gyrus (BA 6) 6 24 69 3.9 19Right precentral gyrus (BA 4) 24 24 72 3.6 11Right precuneus (BA 7) 3 33 54 3.7 13Left precuneus (BA 7) ... cuneus (BA 30) 6 57 15 4.7 48Right cuneus (BA 18) 6 87 24 3.7 6.

15 Sep 2006: There is also. [Journal of Petrologf, Vol. 29, P t n 3, pp 599-«24, 1988] Oxford Umvcroty Prcu 19S8. ... FJH,. (24). We determined numerical solutions of (15)—(18) in addition to either (19)—(23) or merely (24).The differences were negligible.

26 Apr 2006: The boundaryconditions at t'0 are Eq. (12),. h"0 (z"f(t)) (23). [h]ml "0 (z"f(t)), (24). ... Wettlaufer, M.G. Worster, H.E. Huppert, Geophys. Res. Lett. 24 (1997) 1251.[12] D.L.