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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.

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.

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.

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.

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.

30 May 2006: 1. oo 1.712 1.26 1.42 1.10 1.24. 13.61 1.200 0.79 1.06 1.

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).

13 Nov 2006: 3(b). The AFM analysis shows a w of 40,200 and 100 nm for a respective original 0.3-, 1- and 5-nmFe thickness (Figs. ... Annealing in pure NH3 (200 sccm, 0.6 mbar pressure) at500 C results in a distinctively different topography for all Fethicknesses.

6 Dec 2006: 5 ] to films deposited. by cathodic arc systems. Doping in ta-C can only bedecreases from 300 cm1 to 200 cm1 for temperaturesbetween room temperature and 200C.

22 Nov 2006: It reaches 200 eV at 1.39104mbar. The trend observed in Ar plasma is expected to be. ... Tencor Alpha-step 200 profilometer. A series of six. measurements along two perpendicular directions in the.

19 Apr 2006: 1984). This excess emission comes from dust in orbitaround the stars and its relatively cold temperature implies thatit resides at large distances from the stars, 30–200 AU, some-thing which ... 2003a) and IRAS observations at 60 and 100 µmhad 3σ

12 Oct 2006: For example, if d0 = 1, d1 = 10, d2 = 1and d3 = 10, the calculation (M1M2)M3 requires 20 scalar multiplications, butthe calculation M1(M2M3) requires 200 scalar multiplications.

26 Jan 2006: A lossof 100–200 l is usually observed. Purification of Dynamin and Its Mutants from E. ... Scale bars are 200 nm in. length. [52] IN VITRO RECONSTITUTION OF ENDOCYTIC STAGES 607.

20 Jan 2006: It got its name from ancient tree stumps, and for over 200 years has been popular with collectors for its copious fossils - mammoth, sabretooth cat, bison and other exotic creatures. ... The implications are huge. If evidence for hominins 700,000 years

27 Apr 2006: Fig. 1. The velocity of the head is approximately constant for a distance of about 200 cm, which is approximately ten times the lock. ... 3. Over the first 1.5 m the three. 500. ' 200.

23 Feb 2006: 18 Y. WESLEY WONG AND SERGIO PELLEGRINO. 0 50 100 150 200-1. ... 20, 200–207, 227–233, 256–262, 279-284. [Wong 2003] Wong, Y. W., 2003.