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. Galaxies and matter in the universe clump in an intricate network of filaments and voids, known as the Cosmic Web. 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.
An international team of researchers is studying this issue within the Constrained Local UniversE Simulations project (CLUES) that use the observed positions and peculiar velocities of galaxies within Tens of Millions of light years of the Milky Way to accurately simulate the local environment of the Milky Way.
"The main goal of this project is to simulate the evolution of the Local Group - the Andromeda and Milky Way galaxies and their low-mass neighbours - within their observed large scale environment", said Stefan Gottlöber of the Leibniz Institute for Astrophysics Potsdam.
The image below shows a Cosmic Web Stripping removes gas from a very fast dwarf galaxy crossing the local web. The image is a visualization of a CLUES simulation. The arrow symbolizes the velocity oft he dwarf, located right below. 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.
The study of Benítez Llambay and colleagues is published in the February issue of Astrophysical Letters. More information: Benítez-Llambay, A. et al. Dwarf galaxies and the Cosmic Web, Astrophysical Letters. doi:10.1088/2041-8205/763/2/L41.
The image at the top of the page shows a small galaxy, UGC 5288, 16 million light-years from Earth surrounded by a huge disk of hydrogen gas that has not been involved in the galaxy's star-formation processes and may be primordial material left over from the galaxy's formation captured by the National Science Foundation's Very Large Array (VLA) radio telescope.
Image credit: Alejandro Benítez Llambay
Source: The Daily Galaxy via Leibniz Institute for Astrophysics Potsdam