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27 Apr 2006: 8 c ) and is graphed in Fig. 5. 200 -. 160 h(m). 120. 8 0 -. 4 0 -. 107. o ,6o 26o 36o r(m). ... t f o r d i s c u s s i o n ). 0 200 400 600 Metres I i I. SCALE. Fig. 9.

18 Sep 2006: In t h e case o f olivine, the best available estimate of L is 200 cal g m - 1 (Bottinga a n d Richet 1978), a n d ... 3. 100. o. z 200. I 0 I 0 0 I 0 0 0.

19 Apr 2006: 200 100 0 -100 -200RA offset, AU. -200. -100. 0. 100. ... 200. Dec. off. set,. AU. FIGURE 5. Impact of the outward migration of a Neptune mass planet on a planetesimal disk aroundVega [27]: orbital distribution of planetesimals at the beginning (top

26 Apr 2006: 1125WETTLAUFER ET AL.: SOLIDIFICATION OF LEADS. profile was taken after the buoy had reached the oceanic tem-perature, and each subsequent profile is separated by 200 min.A quantitative analysis of ... The initial profile was taken after the buoy had

15 Sep 2006: 400. 300. 200. a). BS. 100 2O0 300. TIME (yre). S! ... 100. 400. b). 100 200. TIME (yre). 300 4OO. FIG 5 Variations of (a) temperature, and (b) thickness of the silicic magma layer with time for a 500 m thick sillemplaced

30 May 2006: directEntries 2000000Mean -0.02588. RMS 17.87. -600 -400 -200 0 200 400 6001. ... directEntries 2000000Mean -0.02588. RMS 17.87. badEntries 2000000Mean 0.01601. RMS 7.586. -600 -400 -200 0 200 400 6001.

13 Nov 2006: process gas at a flow rate of 100–200 sccm. A 2.45 GHz. ... microwave discharge is ignited for 1–3 s at a power of 200–.

19 Apr 2006: HD207129 G0V 15.6 1.0 104 Spline 603022901660 8. HD22049 ǫ Eri K2V 3.22 1.1 104 Best fit model 730 200 10HD39060 β Pic A5V 19.3 3 ... HD109085 0.0 4.2 4.0 180 40HD38393 0.0 2.7 0.4 200 50HD48682 0.0 2.3 7.0 71 15a.

28 Nov 2006: Acetyl Transferase Assays. GST-MEK2 (0.5 g) (purified by usingstandard protocols for GST-tagged protein purification) wasincubated with varying amounts (0 –200 ng) of (His)6-YopJ-wt ... Stimulation of MEK and Erk phosphorylation by various

21 Sep 2006: Furthermore, since the size of the ROIs may vary from one videoto the other, the final MGO images are resized to the corresponding refined images withstandard size (which is 200 200 ... 3.2 Dimension Reduction by PCA. In order to reduce the number of

28 Jul 2006: as to be expected, the figure is much lower for the 200 journals with highest cumulative impact.

13 Nov 2006: Scale bars: (a) 200 nm,(b) 1 μm. show that in most cases just a few nanofibres grow from eachdot. ... spectralregion, and scanning the samples with steps of 200 and 400 nm,respectively.

27 Nov 2006: Robertson. 0. 100. 200. 300. 400. GT1060 cm1. 633 nm. 514.5 nm. ... 0. 100. 200. 300. 80 100 120 140 160. 1.0. 1.5.

30 May 2006: Y f 5 200 -. 6 a. 250 -. 300 -. Salinity ( % o ). I I I I I I I I 34.2 34.3 3 4 4 34.5 34.6 34.7 ... 200. n E. 300. 350. I I 0.1 OC. FIGURE 8.

21 Sep 2006: 0 50 100 150 200 250 300 350 4000.25. 0.2. 0.15. ... Fea. ture. Val. ueBatch OSMINC OSM. 50 100 150 200 250 300 350 4000.

5 May 2006: Details of our finite-difference numericalcode are presented the Appendix. We used a mesh of 320 horizontal and 200 verticalintervals.

19 Apr 2006: up to 200 km in diameter) for impacts with a range ofimpact parameters and with relative velocities comparable to thoseexpected in extrasolar planetesimal discs. ... 6b), all models predict a lifetimethat is shorter than the age of the system (200 Myr)

19 Apr 2006: Compared to the fullextent of the mid-IR–emitting size of the disk (200 AU), therelatively small values of the dust FWHM sizes suggest thatthe mid-IR emission is sharply peaked ... extends out to at least a radius of 100 (200 AU) fromthe star in the

6 Dec 2006: 150 C, 200 C, 250 C, and 300 C at various nitgen pressures. ... Above 200 Cconductivity becomes almost independent of N contentits dependence on temperature declines.

19 Apr 2006: Fitting a Gaussian to therebinned 850 m data indicates that the 850 m emission has aFWHM of 19B4 0B2 and is centered on the star to within 200. ... the disk around star Fomalhaut, which has anage of 200 Myr (Wyatt & Dent 2002).