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Chandler, Harry

The Wonderful Tar Baby Story Joel Chandler Harris, 1848-1908... [Pg.169]

Tagge EP, Chandler J, Harris B, Czako M, Marton L, Willingham MC, Burbage C, Afrin L, Frankel AE (1996) Protein Exp Purif 8 109... [Pg.154]

Because density fluctuations produce a long-lived perturbation, whereas collisional dynamics are fast, the Raman echo is a definitive experiment for testing this prediction. An excellent system for this test is the sym-methyl stretch of acetonitrile (3). There have been many Raman line shape studies of this mode, which concluded that the IBC theory of collisional dynamics alone can account for the linewidth (84,90,91,133,134). On the other hand, calculations by George and Harris using Schweizer and Chandler s theory predicted that a substantial fraction of the linewidth is due to density fluctuations (135). [Pg.427]

Harris SR, Swanson MW, Andrews MS, Sells CJ, Robinson NM, Bennett EC, Chandler LS. 1984. Predictive validity of the movement assessment of infants. J Dev Behav Pediatr 5 336-342. [Pg.153]

Jasty M, Bragdon C, Jiranek W, Chandler H, Maloney W, Harris WH. Etiology of osteolysis around porous-coated cementless total hip arthrt lasties. Clin Orthop Relat Res 1994(308) 111-26. [Pg.431]


See other pages where Chandler, Harry is mentioned: [Pg.100]    [Pg.102]    [Pg.285]    [Pg.159]    [Pg.659]    [Pg.749]    [Pg.713]   
See also in sourсe #XX -- [ Pg.159 ]




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