- #1
Saul
- 271
- 4
This is a significant discovery that something is fundamentally controlling and ordering the properties of spiral and disk gaseous galaxies. Elliptical galaxies have no gas and no star formation.
The question is not only what but how is the unknown parameter controlling spiral and disk galaxy evolution and properties.
This appears to me to be a discovery as significant as the Hertzsprung-Russell diagram which led to the formation theory of stars.
http://en.wikipedia.org/wiki/Hertzsprung–Russell_diagram
http://arxiv.org/abs/0811.1554
http://www.nature.com/nature/journal/v455/n7216/abs/nature07366.html
The question is not only what but how is the unknown parameter controlling spiral and disk galaxy evolution and properties.
This appears to me to be a discovery as significant as the Hertzsprung-Russell diagram which led to the formation theory of stars.
http://en.wikipedia.org/wiki/Hertzsprung–Russell_diagram
http://arxiv.org/abs/0811.1554
http://www.nature.com/nature/journal/v455/n7216/abs/nature07366.html
Galaxies (my comment: Spiral and disk) appear simpler (my comment tightly controlled) than expected
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 holes1. The hierarchical theory of galaxy formation holds that galaxies are assembled from smaller pieces, through numerous mergers of cold dark matter2, 3, 4. 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 from optical selection effects5, shows five independent correlations among six independent observables, despite having a wide range of properties. This implies that the structure of these galaxies must be controlled by a single parameter, although we cannot identify this parameter from our data set. Such a degree of organization appears to be at odds with hierarchical galaxy formation, a central tenet of the cold dark matter model in cosmology6.
If, as we have argued, galaxies come from at most a six-parameter set, then for gaseous galaxies to appear as a one-parameter set, as observed here, the theory of galaxy formation and evolution must supply five independent constraint equations to constrain the observations. This is such a stringent set of requirements that it is hard to imagine any theory, apart from the correct one, fulfilling them all. For instance, consider heirarchical galaxy formation in the dark matter model, which has been widely discussed in the literature3,4. Even after extensive simplification, it still contains four parameters per galaxy: mass, spin, halo-concentration index and epoch of formation. Consider spin alone, which is thought to be the result of early tidal torquing. Simulations produce spins, independent of mass, with a log-normal distribution. Higher-spin discs naturally cannot contract as far; thus, to a much greater extent than for low-spin discs, their dynamics is controlled by their dark halos, so it is unexpected to see the nearly constant dynamical-mass/luminosity ratio that we and others14 actually observe. Heirarchical galaxy formation simply does not fit the constraints set by the correlation structure in the Equatorial Survey.
More generally, a process of hierarchical merging, in which the present properties of any galaxy are determined by the necessarily haphazard details of its last major mergers, hardly seems consistent with the very high degree of organisation revealed in this analysis. Hierarchical galaxy formation does not explain the commonplace gaseous galaxies we observe. So much organization, and a single controlling parameter which cannot be identified for now argue for some simpler model of formation. It would be illuminating to identify the single controlling galaxy parameter, but this cannot be attempted from the present data.
It is natural to ask why this fundamental line was not discovered before. To some extent it was because even the pioneers24,25 and others26,27,28 working with small numbers of optically selected spirals could reduce six observables to two; one relating to size, one to morphology. The strong optical selection effects, which hamper optical astronomers in detecting and measuring galaxies whose surface brightnesses are barely brighter than the sky5,29, disguised galaxies’ simplicity.