A seemingly impossible cluster of more than 30 galaxies crammed into a volume just 500,000 light-years across has been found in the universe just 1.4 billion years after the Big Bang — and with a temperature that breaks all the rules.
The discovery, by astronomers using Chile’s Atacama Large Millimeter/submillimeter Array (ALMA), of the galaxy cluster labeled SPT2349-56 challenges our understanding of how quickly galaxies and galaxy clusters were able to form.
Galaxy clusters are filled with a fog of hot gas that we call the intracluster medium — what Dazhi Zhou, who is a PhD candidate at University of British Columbia in Canada and lead author of the paper describing the findings, refers to as a galaxy cluster’s ‘atmosphere’. In most clusters, the intracluster medium can reach tens or even hundreds of millions of degrees Celsius.
Astrophysicists thought that it would take many billions of years for the intra-cluster medium to grow so hot, but SPT2349-56 suggests otherwise.
The intracluster medium temperature of SPT2349-56 was measured indirectly via what’s called the Sunyaev–Zeldovich effect, whereby galaxy clusters leave their mark on the cosmic microwave background (CMB) radiation, which is the leftover heat from the Big Bang. As CMB photons enter the cluster, they gain an energy boost by scattering off electrons within the intra-cluster medium. The hotter the medium, the more the electrons are moving and therefore the greater the energy boost they pass onto the CMB photons when the photons interact with the electrons. This energy boost can then be seen in the CMB corresponding to the location of a given cluster.
More distant clusters that existed earlier in the universe than SPT2349-56 have previously been discovered.
The difference between these clusters and SPT2349-56 is that the earlier clusters are designated ‘protoclusters’, meaning that they are not yet fully gravitationally bound. According to our best models of how galaxy clusters form, the gas in the intra-cluster medium becomes heated by the dynamical collapse of the galaxies into a stable, gravitationally bound state.
As such, these protoclusters do not yet have high intra-cluster medium temperatures and the models suggest that they won’t reach high temperatures for many billions more years. SPT2349-56, on the other hand, seems to have rushed ahead, suggesting that our models of how galaxy clusters grow and become so hot are incomplete.
What SPT2349-56 and the earlier protoclusters all have in common is frenetic star formation. The size of SPT2349-56 is about the same as the halo of old stars and dark matter that surrounds our Milky Way galaxy, so the 30 or more galaxies that are members of SPT2349-56 are small. However, they won’t remain small for long. Within those galaxies the stars are forming at a rate five-thousand times faster than in our Milky Way galaxy where on average less than ten stars form each year.
(Yahoo! News)
