Dust may be more rare than expected in galaxies of the early Universe making them much more difficult to observe, according to an international research team. In a galaxy named IZw 18, which has a chemistry that is more like galaxies of the very early Universe with a very low abundance of metals and a lot of gas in the form of hydrogen, the team measured the lowest dust mass of a galaxy that has ever been measured.
The galaxy, I Zw 18, is nearby, which makes it easier to study, but has properties that are very similar to galaxies of the high redshift Univese.
"It's an extreme galaxy in the local Universe, but it tells us a lot about a stage that almost all galaxies have gone through, so it gives us a picture of what the first galaxies look like."
"This means, firstly, that they will look different than we expect and make different populations of stars than we expect. And secondly, that they will be much more difficult to observe, even with state-of-the-art facilities being built now such as the Atacama Large Millimeter/sub-millimeter Array (ALMA) of radio telescopes in northern Chile.
"IZw 18 is typical of very high redshift galaxies because it is very actively forming stars, and has a chemistry that is more like galaxies of the very early Universe with a very low abundance of metals and a lot of gas in the form of hydrogen," he said.
"Our result implies that current theories to describe the formation of stars when the Universe was very young are incomplete, and are built on invalid assumptions."
According to Dr Fisher, the amount of dust is very important for the formation of stars. "What we think is going on, is that the harsh environment inside the galaxy we examined is adversely affecting the amount of dust in it. The radiation field measured inside I Zw 18 was roughly 200 times stronger than what we experience here in the Milky Way." Dr Fisher said that based on the findings, theories should be amended to account for environment in making stars.
The team included researchers from the University of Maryland, Swinburne University of Technology, Princeton University, Max-Plank Institut für Astronomie, Germany; National Radio Astronomy Observatory, Virginia; Department of Physics and Astronomy, Macalester College, Saint Paul, Minnesota.
The Daily Galaxy via Swinburne University and Nature