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C NMR spectrum of polyplperylene Polymer A ,

C NMR spectrum of Pt Ru-35 obtained in 14.1 T field. Dotted lines represent the double-Gaussian deconvolution that indicates the presence of two peaks, corresponding to the two different CO populations.

C NMR spectrum of Pt Ru-3S obtained in 14.1 T ficW-Dotted lines represent the double-Gaussian deconvolution that indicates the presence of two peaks, corresponding to the two dilTetent CO populations.

C NMR spectrum of PTo. PTo gives two sharply resolved absorption bands at 124.8 ppm FWHM

C NMR spectrum of triethyleneglycol

C NMR spectrum of34 , inset

C NMR spectrum ofCso, Buckminsterfullerene. f CNMR spectrum of a mixed sample in which is much reduced, c C NMR spectrum of Cm, fullerene-70. The line assignments given are based on the observed intensities and semi-quantitative strain arguments, and are subject to confirmation. The wing of the intense benzene solvent signal lies at the far right hand side

C NMR spin-diffusion spectrum of products of the conversion of meth-

C Noiisdectivc image without water suppression of the same slice. The held of view is 4cm X 4 cm. Adapted from IRumI I with permission from Elsevier Science.

C Nonlinear emission spectra measured from

C NQS and CP MAS NMR spectra of hypercrosslinked polystyrene resin .

C ns tu PHIPspectrum after hydrogenation with para-hydrogen and polarisation transfer from protons to carbons. Note the extremely high signal noise ratio in the single shot spectrum, which is a measure for the strong signal enhancement obtained by PHIP .

C NTi values for methionine-enkephalin.

C nuclear magnetic resonance spectrum of chlorpromazine hydrochloride.

C nuclear magnetic resonance spectrum of indinavir sulfate.

C Nuclear magnetic resonance spectrum of lipids extracted from the shed skin of a pregnant female Crotalus v. viridis.

C nuclear magnetic resonance spectrum of procaine .

C o 5 mM. Reproduced from Goto, A. Fukuda, T. Macromolecules Mil, 30,5183-5186, with permission from the American Chemical Society.

C O abundance ratios . Open symbols-, irregular galaxies filled symbols

C O and O H gradients in M101 . Left panels

C o grafting on the P3HT rod-coil copolymer 12

C O ratio vs. O H in Galactic and extragalactic H n regions, based on International Ultraviolet Explorer .

C o solubility is invariant under effect of the methyl groups located in the meta-positions of the benzene core.

C O vs. in stars, after Akerman et at. and references therein, with an additional point representing a damped Lyman-a system at a high redshift. The broad trend is in fair agreement with the H n region results shown in

C O vs. O H in stars and H n regions, from various sources. Curves A, B and C correspond to increasing star-formation efficiencies .



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