Morphological complexity of NGC 628 - a multiwavelength multiscale analysis using the ordinal pattern framework
Athokpam Langlen Chanu, S Amrutha, Pravabati Chingangbam, Changbom Park

TL;DR
This study applies the ordinal patterns framework to analyze the morphological complexity of galaxy NGC 628 across multiple wavelengths and scales, revealing a characteristic 200 parsec transition scale and universal statistical behavior.
Contribution
It introduces a multiscale, multiwavelength analysis of galactic morphology using ordinal pattern statistics, highlighting a universal behavior in large-scale structures.
Findings
Identified a ~200 parsec scale marking structural transition.
Observed convergence of $C$ vs. $H$ trajectories toward a universal attractor.
Detected consistent statistical behavior across different wavelengths.
Abstract
As statistical systems, galaxies exhibit a rich interplay between organized structure and stochastic fluctuations across a broad range of spatial scales. This duality motivates the need for quantitative frameworks capable of capturing their morphological complexity. The ordinal patterns framework, along with its associated statistical measures: permutation entropy (), disequilibrium (), statistical complexity (), and ordinal network node entropy, has recently emerged as a powerful tool for analyzing such complexity in physical systems. We apply this framework in a multiwavelength, multiscale analysis of the galaxy NGC 628, utilizing observations in the near-ultraviolet, near-infrared, mid-infrared, and millimeter bands. Our results reveal a characteristic spatial scale of approximately 200 parsecs, marking the transition from small-scale structures influenced by star…
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