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arX iv:0 704. 0873 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf18 Apr 2007: 200. 7. Mon. Not. R. Astron. Soc. 000, 1–6 (2006) Printed 9 April 2007 (MN LATEX style file v2.2). ... Doppler systems arepredicted here to form from 5-200 Jupiter masses of gas inthe disk, enough to make gas giant planets. -
seminar.dvi
www.statslab.cam.ac.uk/~rrw1/talks/binpacking.pdf18 Jan 2007: PAIRS j;k FOR WHICH FFD HAS LINEAREXPECTED WASTE UNDER Ufj;kg0 100 200 300 400 500. ... 0. 50. 100. 150. 200. 250. k. j. FFD RESULTSTHEOREMIf j < k1=2 then the expected waste for FFD is O(1).THEOREMThere exist pairs j;k with j arbitrarily large -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2.pdf5 Jun 2007: a factor of 200:1 based onthe well established space densities of the foreground L and T dwarfs. ... Observing efficiency % per tile - - 73.3 - 69.9Time for 8,200 sq deg = 5467 tiles of 1.5 sq degTotal Elapsed Hours - - 373 - 391. -
Pupils in Northern Ireland learn about life at Cambridge | University …
https://www.cam.ac.uk/news/pupils-in-northern-ireland-learn-about-life-at-cambridge19 Mar 2007: A total of 200 pupils from 34 schools as far afield as Belfast, Enniskillen and Newry will be spending the morning at Cookstown High School on Tuesday, March 20. -
journal.dvi
mi.eng.cam.ac.uk/~mjfg/kcs_csl.pdf4 Apr 2007: observationMPE trajectoryfMPEMPE trajectory. 50 100 150 200 250 3000.2. 0.1. 0. ... Dev. of pMPE trajectory. 50 100 150 200 250 300. 0.8. -
finitet4.dvi
www.damtp.cam.ac.uk/user/ngb23/publications/finitet4.pdf24 Aug 2007: 100 200 300 400 500 600. 500. 1000. 1500. 2000. 2500. ... T /Tλ. 0 200 400 600 8000. 100. 200. 300. 400. -
Proceedingsofthe E-MRS 2006 Symposium E: Scienceand Technologyof…
www-g.eng.cam.ac.uk/nms/publications/pdf/Ferrari_PE2007.pdf30 Mar 2007: Calleja 200. Electronic properties of InAs/GaAs nanowire superlattices. Y.M. Niquet 204. ... Calleja, E. 200. Canc-ado, L.G. 88. Cantoro, M. 1. Carbone, L. -
LETTERS Breakdown of the adiabaticBorn–Oppenheimer approximationin…
www-g.eng.cam.ac.uk/nms/publications/pdf/Pisana_NM2007.pdf2 Mar 2007: Acc. Chem. Res. 35, 193–200 (2002).7. Alfe, D., Gillan, M. J. & ... Nature 438,. 197–200 (2005).16. Zhang, Y., Tan, Y. W., Stormer, H. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf5 Jun 2007: The Y-J colour is ESSENTIAL since the so called ’rare’ L and T dwarfs outnumberthe quasars by a factor of 200:1 based on the well established space densities of ... Observing efficiency % per tile 73.3 76.1 - - 69.9. Time for 8,200 sq deg = 5467 -
Inclined to exchange:shocking gravity currents John Hinch (DAMTP) and …
www.damtp.cam.ac.uk/user/hinch/talks/nottingham.pdf19 Nov 2007: 0.742 0.789 0 < t < 200. Slow logarithmic approach also in experimental data.
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