Search

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

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.

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

19 Apr 2006: 20. -10. 0. 10. 20. Dec. off. set,. arcs. ec. É6 200 100 0 -100 -200RA offset, AU. ... 200. -100. 0. 100. 200. Dec. off. set,. AU. Î: Ì î Ï?Ð «0£sU6¤0 09¢&£¤¢?_M«XÓ¢ 9ªsM«ºs¤Ò_Ü£MX?ß 6_ºs_ºs_¡Çà Í

3 Nov 2006: 150. -100. -50. 0. 50. 100. 150. 200. 250. 300. Left Lateral Right Lateral. ... BehavNeurol 12:191--200. Shulman GL, Fiez JA, Corbetta M, Buckner RL, Miezin FM, Raichle ME,Petersen SE.

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.

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.

21 Sep 2006: Dense rings at 200 and 325 AU with tightly wound spiral structure (Clampin et al.

19 Apr 2006: Not Avail. no 16HD 107146 G2 30-250 130 red (V-I) 0.3 0.1 yes 17,18Fomalhaut A3 200 140 Not Avail. ... Emission (Additional)Vega A0 200 >90 23,24,25 Eridani K2 <1000 60 26,27η Corvi F2 1000 100 28τ Ceti G8 5000 55 29.

23 Nov 2006: UNIVERSITY OF CAMBRIDGE. Department of Applied Mathematics and Theoretical Physics. Numerical Solution of Differential Equations. A. Iserles. Part III. Michaelmas 2007. Numerical Analysis Group. Centre for Mathematical SciencesWilberforce Rd.

6 Jun 2006: Execute tiles that overlap with 200 deepest XMM pointings. • Fornax galaxy cluster(50deg2). ... The black filled circles are 200 deep public XMM pointings from the 2XMMcatalogue.

27 Apr 2006: Fluid Mech. 33 (1968) 183-200. 16 H.E. H u p p e r t and P.F.

13 Nov 2006: lecular weight) aqueous solution and ultrasonicated again for 40 minutes at 200 W. ... The corre-. sponding SWNTs-PVA composite has a broad absorption band (FWHM 200 nm) centred at 1530 nm.

30 May 2006: A. Hallworth. I I I 0 50 200 300 400 500. ... Time (min). I. 0 50 200 300 400 500. Time (min).

13 Nov 2006: We use polished, 0.01-0.02 cm boron-doped Si(100)wafers as substrates, covered with thermally grown SiO2(50-200 nm). ... The process temperature is indicatedfor each sample. Scale bars: 100 (b-d), 500 (e), and 200 nm (f).

5 May 2006: Perspex, 1.1 cm thick, with internal lengths and depths of 50 cm 30 cm, 200 cm 22.3 cm and 232.5 cm 40 cm.

19 Apr 2006: Dust emissionpeaks are resolved with source sizes of 200 to 500 (1.7 104 to4.3 104 AU).

13 Nov 2006: Then, pure SiH4was admitted as the Si source gas, the total pressure vary-ing between 200 mTorr and 10 Torr. ... arrow). Scale bar: 1 µm. much thicker (200–300 nm) and tapered, indicating that Siovergrowth on the NW side walls also occurred during

17 May 2006: Liquid rope coiling 289. 0.6. 0.8. 1.0. 0.8. 1.0. 100 200 500 1000 2000 5000.