Sunday, February 03, 2013

Astronomers Ask 'Where Are All the Dwarf Galaxies?'

Could these unseen dwarf galaxies be "dark matter"?
"Dark matter" is believed to exist to explain the fact that the expansion of the universe seems to be speeding up. But as far as I can tell, all of the evidence I have seen could be a result not of an increasingly expanding universe, but of the effects of unseen regular matter on light, either thru causing a red shift or by blocking out some of the light.

http://www.sciencedaily.com/releases/2013/02/130201090359.htm

Feb. 1, 2013 — Astronomers of the international CLUES collaboration have identified "Cosmic Web Stripping" as a new way of explaining the famous missing dwarf problem: the lack of observed dwarf galaxies compared with that predicted by the theory of Cold Dark Matter and Dark Energy.

High-precision observations over the last two decades have indicated that our Universe consists of about 75% Dark Energy, 20% Dark Matter and 5% ordinary matter.

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Computer experiments on massive supercomputers have shown that in such a Universe a huge number of small "dwarf" galaxies weighing just one thousandth of the Milky Way should have formed in our cosmic neighbourhood. Yet only a handful of these galaxies are observed orbiting around the Milky Way. The observed scarcity of dwarf galaxies is a major challenge to our understanding of galaxy formation.

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Analysing the CLUES simulations, the astronomers have now found that some of the far-out dwarf galaxies in the Local Group move with such high velocities with respect to the Cosmic Web that most of their gas can be stripped and effectively removed. They call this mechanism "Cosmic Web Stripping," since it is the pancake and filamentary structure of the cosmos that is responsible for depleting the dwarfs' gas supply.

"These dwarfs move so fast that even the weakest membranes of the Cosmic Web can rip off their gas," explained Alejandro Benítez LLambay, PhD student at the Instituto de Astronomía Teórica y Experimental of the Universidad Nacional de Córdoba in Argentina, and first author of the publication of this study. Without a large gas reservoir out of which to form stars, these dwarf galaxies should be so small and dim that they would be hardly be visible today. The missing dwarfs may simply be too faint to see.

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