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The interstellar medium seems to have an underlying fractal structure which can be characterized through its fractal dimension. However, interstellar clouds are observed as projected two-dimensional images, and the projection of a…

天体物理学 · 物理学 2007-05-23 Nestor Sanchez , Emilio J. Alfaro , Enrique Perez

There exists observational evidence that the interstellar medium has a fractal structure in a wide range of spatial scales. The measurement of the fractal dimension (Df) of interstellar clouds is a simple way to characterize this fractal…

天体物理学 · 物理学 2011-02-11 Nestor Sanchez , Emilio J. Alfaro , Enrique Perez

The Interstellar Medium seems to have an underlying fractal structure, which can be characterized through its fractal dimension (Df). However, several factors may affect the determination of Df, such as distortions due to projection, low…

天体物理学 · 物理学 2008-03-11 Nestor Sanchez , Emilio J. Alfaro , Enrique Perez

Observations of interstellar gas clouds are typically limited to two-dimensional (2D) projections of the intrinsically three-dimensional (3D) structure of the clouds. In this study, we present a novel method for relating the 2D projected…

星系天体物理 · 物理学 2019-06-05 James R. Beattie , Christoph Federrath , Ralf S. Klessen

Clouds in observations are fractals: they show self-similarity across scales ranging from one to 1000 km. This includes individual storms and large-scale cloud structures typical of organised convection. It is not known whether global…

大气与海洋物理 · 物理学 2022-01-05 Hannah M. Christensen , Oliver G. A. Driver

The fractal dimension $D$ is used to map the large-scale galaxy distribution in the Universe by color types: blue, green and red. Using a $NUVrK$-complete COSMOS2020 subsample of 618,952 galaxies observed up to $z=4$, number densities were…

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…

星系天体物理 · 物理学 2020-08-04 Canavesi Tobias , Hurtado Santiago

Most of the known methods for estimating the fractal dimension of fractal sets are based on the evaluation of a single geometric characteristic, e.g. the volume of its parallel sets. We propose a method involving the evaluation of several…

度量几何 · 数学 2015-06-22 Evgeny Spodarev , Peter Straka , Steffen Winter

Quantitative analysis of the structure of star clusters is crucial for understanding their formation and evolution. In this article, we explore the application of fractal dimension analysis to study the evolution of star clusters, also…

星系天体物理 · 物理学 2025-07-01 N. Ussipov , A. Akhmetali , M. Zaidyn , A. Akniyazova , A. Sakan , M. Kalambay , B. Shukirgaliyev

Estimates of the fractal dimension $D$ of the set of galaxies in the universe, based on ever improving data sets, tend to settle on $D\approx 2$. This result raised a raging debate due to its glaring contradiction with astrophysical models…

天体物理学 · 物理学 2007-05-23 Jean-Pierre Eckmann , Esa Järvenpää , Maarit Järvenpää , Itamar Procaccia

Fractals are a basic tool to phenomenologically describe natural objects having a high degree of temporal or spatial variability. From a physical point of view the fractal properties of natural systems can also be interpreted by using the…

高能天体物理现象 · 物理学 2015-05-28 C. S. Leung , J. Y. Wei , A. K. H. Kong , Z. Kovács , T. Harko

The multifractal geometry remains an under-exploited approach to describe and quantify the large-scale structure of interstellar clouds. In this paper, the typical tools of multifractal analysis are applied to Herschel far-infrared (70-500…

星系天体物理 · 物理学 2018-08-09 D. Elia , F. Strafella , S. Dib , N. Schneider , P. Hennebelle , S. Pezzuto , S. Molinari , E. Schisano , S. E. Jaffa

We present a review of the history and the present state of the fractal approach to the large-scale distribution of galaxies. Angular correlation function was used as a general instrument for the structure analysis. It was realized later…

天体物理学 · 物理学 2007-05-23 Yurij Baryshev , Pekka Teerikorpi

The fractal dimension of a surface allows its degree of roughness to be characterized quantitatively. However, limited effort is attempted to calculate the fractal dimension of surfaces computed from precisely known atomic coordinates from…

数学软件 · 计算机科学 2024-03-12 Jonathan Yik Chang Ting , Andrew Thomas Agars Wood , Amanda Susan Barnard

It is known that the gas has a fractal structure in a wide range of spatial scales with a fractal dimension that seems to be a constant around Df = 2.7. It is expected that stars forming from this fractal medium exhibit similar fractal…

天体物理学 · 物理学 2009-06-23 Nestor Sanchez , Emilio J. Alfaro

Fractal surfaces are ubiquitous in nature as well as in the sciences. The examples range from the cloud boundaries to the corroded surfaces. Fractal dimension gives a measure of the irregularity in the object under study. We present a…

地球物理 · 物理学 2014-12-10 Kiran M. Kolwankar , Nakul N. Karle

The fractal structure of real world objects is often analyzed using digital images. In this context, the compression fractal dimension is put forward. It provides a simple method for the direct estimation of the dimension of fractals stored…

图形学 · 计算机科学 2016-08-15 P. Chamorro-Posada

This study builds a bridge between two well-studied but distant topics: fractal dimension and Discrete Global Grid System (DGGS). DGGSs are used as covering sets for geospatial vector data to calculate the Minkowski-Bouligand dimension.…

计算工程、金融与科学 · 计算机科学 2025-06-24 Pramit Ghosh

We analyze the fractal dimension of open clusters using 3D spatial data from Gaia DR3 for 93 open clusters from Pang et al. (2024) and 127 open clusters from Hunt & Reffert (2024) within 500 pc. The box-counting method is adopted to…

星系天体物理 · 物理学 2025-03-05 Chang Qin , Xiaoying Pang , Mario Pasquato , M. B. N. Kouwenhoven , Antonella Vallenari

Three-dimensional fractal models on grids of 200**3 pixels are generated from the inverse Fourier transform of noise with a power law cutoff, exponentiated to give a log normal distribution of density. The fractals are clipped at various…

天体物理学 · 物理学 2009-11-07 B. G. Elmegreen
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