Can fractal dimension distinguish between grand-design and flocculent spiral arms?
Biju Saha, Subhadip Dutta, Arunima Banerjee

TL;DR
This study demonstrates that fractal dimension effectively distinguishes between grand-design and flocculent spiral galaxies, correlates with galaxy properties, and offers insights into spiral arm formation mechanisms.
Contribution
Introduces fractal dimension as a novel, non-parametric metric for classifying spiral galaxy morphology and compares its effectiveness with other parameters.
Findings
Fractal dimension differs significantly between galaxy types.
Fractal dimension has higher feature importance than traditional metrics.
Anti-correlation between fractal dimension and central velocity dispersion.
Abstract
About two-thirds of disk galaxies host spiral arms, ranging from well-delineated grand-design spirals to fragmented flocculent spiral galaxies. We introduce fractal dimension as a non-parametric measure to distinguish between grand-designs and flocculents. We calculate the of 197 grand-designs and 322 flocculents from SDSS DR18, using the samples of \citet{Buta..2015} and \citet{Sarkar..2023}. Our calculated median values of are and for the grand-designs and flocculents, respectively. In addition, a Kolmogorov-Smirnov (K-S) test rejects null hypothesis that these distributions are drawn from the same population. Finally, using a Random Forest (RF) model, we compare the effectiveness of in classifying spiral arm morphology, as compared to five other parameters viz. total atomic hydrogen HI mass , ratio of…
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