论文标题
恒星形成区域的分形维度
Fractal dimension in star formation regions
论文作者
论文摘要
螺旋星系中的几项二维研究表明，HII恒星形成区的分形分布，分形尺寸约为2.3。在这项工作中，分形维是通过在R代码中实现的盒子计数方法计算的。作品的创新在于直接在3个维度中计算分形维度，而无需使用GAIA的位置和距离数据（数据版本2）。以银河系研究的区域的估计分形维为2.468（M16），2.126（Orion Nebula）和2.435（RCW 38）。
Several two-dimensional studies in spiral galaxies show that HII star formation regions have a fractal distribution, with a fractal dimension of approximately 2.3. In this work, the fractal dimension is calculated through the box-counting method implemented in an R code. The innovation of the work lies in calculating the fractal dimension directly in 3 dimensions, without the need for the use of projections, using position and distance data from Gaia (Data version 2). The estimated fractal dimension for the regions studied in the Milky Way are 2.468 (M16), 2.126 (Orion Nebula) and 2.435 (RCW 38).
