A Statistical Study of Burns at Saga Medical School Hospital from 1981 to 1991.

1994 ◽  
Vol 56 (3) ◽  
pp. 514-517 ◽  
Author(s):  
Takahisa NISHI ◽  
Kiyohisa MOTOKI ◽  
Yutaka NARISAWA ◽  
Hiromu KOHDA
1993 ◽  
Vol 55 (6) ◽  
pp. 1092-1095 ◽  
Author(s):  
Tatsurou TANAKA ◽  
Kiyohisa MOTOKI ◽  
Takahisa NISHI ◽  
Yutaka NARISAWA ◽  
Hiromu KOHDA

1976 ◽  
Vol 32 ◽  
pp. 675-683
Author(s):  
Keiichi Kodaira

SummaryExcess of [m1] index of Am stars, relative to normal stars, is statistically found to be correlated with rotation velocity; the coefficient is estimated at ∆׀m1׀ /∆V(km/sec) ˜ - 0.0007 among Am stars. This result supports the general view that slow rotation is essential for Am phenomena.


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