PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 47(5) 509-526 1995年 [査読有り]
Previous analyses have revealed that thermodynamic distribution function can represent the galaxy distributions in various observational and numerical data very well. In their analyses, the value of b in the thermodynamic function was used as a fi...
Following recent observational studies of counts-in-cells statistic, we consider the evolution of the third and fourth moments of distribution functions of the density contrast 6. We define a normalized skewness as S = [delta3]/[delta2]2 and a nor...
国際学部
経済学部