Galaxies appear simpler than expected
M. J. Disney, J. D. Romano, D. A. Garcia-Appadoo, A. A. West, J. J., Dalcanton, and L. Cortese

TL;DR
This study reveals that a sample of neutral hydrogen-selected galaxies exhibits strong correlations among their properties, suggesting a single controlling parameter, which challenges the hierarchical galaxy formation model based on cold dark matter.
Contribution
It provides observational evidence that galaxy structures may be governed by a single parameter, contradicting the expected complexity from hierarchical formation theories.
Findings
Five correlations among six galaxy observables
Galaxies appear governed by a single parameter
Challenges hierarchical galaxy formation paradigm
Abstract
Galaxies are complex systems the evolution of which apparently results from the interplay of dynamics, star formation, chemical enrichment, and feedback from supernova explosions and supermassive black holes. The hierarchical theory of galaxy formation holds that galaxies are assembled from smaller pieces, through numerous mergers of cold dark matter. The properties of an individual galaxy should be controlled by six independent parameters including mass, angular-momentum, baryon-fraction, age and size, as well as by the accidents of its recent haphazard merger history. Here we report that a sample of galaxies that were first detected through their neutral hydrogen radio-frequency emission, and are thus free of optical selection effects, shows five independent correlations among six independent observables, despite having a wide range of properties. This implies that the structure of…
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