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相关论文: Fractal dimension of interstellar clouds: opacity …

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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

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

The geometric characteristics of dust clouds provide important information on the physical processes that structure such clouds. One of such characteristics is the $2D$ fractal dimension $D$ of a cloud projected onto the sky plane. In…

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

We study the physical properties derived from interstellar cloud complexes having a fractal structure. We first generate fractal clouds with a given fractal dimension and associate each clump with a maximum in the resulting density field.…

天体物理学 · 物理学 2008-11-26 Nestor Sanchez , Emilio J. Alfaro , Enrique Perez

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

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

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…

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

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

We study the distribution of stars, HII regions, molecular gas, and individual giant molecular clouds in M33 over a wide range of spatial scales. The clustering strength of these components is systematically estimated through the fractal…

宇宙学与河外天体物理 · 物理学 2010-11-08 Nestor Sanchez , Neyda Anez , Emilio J. Alfaro , Mary Crone Odekon

In the interstellar medium, as well as in the Universe, large density fluctuations are observed, that obey power-law density distributions and correlation functions. These structures are hierarchical, chaotic, turbulent, but are also…

天体物理学 · 物理学 2016-08-30 Francoise Combes

The interstellar medium is structured as a hierachy of gas clouds, that looks self-similar over 6 orders of magnitude in scales and 9 in masses. This is one of the more extended fractal in the Universe. At even larger scales, the ensemble…

天体物理学 · 物理学 2018-03-28 F. Combes

Several studies have investigated the fractal and multifractal nature of magnetic features in the solar photosphere and its variation with the solar magnetic activity cycle. Here we extend those studies by examining the fractal geometry of…

天体物理学 · 物理学 2009-11-11 Serena Criscuoli , Mark Rast , Ilaria Ermolli , Mauro Centrone

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

Evidence is presented that the galaxy distribution can be described as a fractal system in the redshift range of the FDF galaxy survey. The fractal dimension $D$ was derived using the FDF galaxy volume number densities in the spatially…

宇宙学与河外天体物理 · 物理学 2014-10-22 G. Conde-Saavedra , A. Iribarrem , Marcelo B. Ribeiro

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

Fractal geometry provides a powerful tool for scale-free spatial analysis of cities, but the fractal dimension calculation results always depend on methods and scopes of study area. This phenomenon has been puzzling many researchers. This…

物理与社会 · 物理学 2019-05-07 Yanguang Chen

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

Sub-millimetre observations suggest that the filaments of interstellar clouds have rather uniform widths and can be described with the so-called Plummer profiles. The shapes of the filament profiles are linked to their physical state.…

星系天体物理 · 物理学 2015-06-05 M. Juvela , J. Malinen , T. Lunttila
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