This image shows the bright emission from carbon and dust in the galaxy surrounding the most distant
Using the IRAM array of millimetre-wave telescopes in the French Alps, a team of European astronomers from Germany, the UK and France has discovered a large reservoir of gas and dust in a galaxy that surrounds the most distant supermassive black hole known. Light from the galaxy, called J1120+0641, has taken so long to reach us that the galaxy is seen as it was only 740 million years after the Big Bang, when the universe was only 1/18th of its current age.
Team leader Dr. Bram Venemans of the Max-Planck Institute for Astronomy in Heidelberg, Germany will present the new discovery on Wednesday 28th March at the RAS / AG National Astronomy Meeting in Manchester, United Kingdom. The Institut de Radioastronomie Millimetrique (IRAM) array is made up of six 15-m size telescopes that detect emission at millimeter wavelengths (about a thousand times as long as visible light) sited on the 2550-m high Plateau de Bure in the French Alps. The IRAM telescopes work together to simulate a single much larger telescope in a so-called interferometer that can study objects in fine detail.
A recent upgrade to IRAM allowed the scientists to detect the newly discovered gas and dust that includes significant quantities of carbon. This is quite unexpected, as the chemical element carbon is created via nuclear fusion of helium in the centres of massive stars and ejected into the galaxy when these stars end their lives in dramatic supernova explosions.
Dr Venemans comments: “It’s really puzzling that such an enormous amount of carbon-enriched gas could have formed at these early times in the universe. The presence of so much carbon confirms that massive star formation must have occurred in the short period between the Big Bang and the time we are now observing the galaxy.”
From the emission from the dust, Venemans and his team were able to show that the galaxy is still forming stars at a rate that is 100 time higher than in our Milky Way. The team give credit to the IRAM upgrade that made the new discovery possible.
“Indeed, we would not have been able to detect this emission only a couple of years ago.” says team member Dr Pierre Cox, director of IRAM.
The astronomers are excited about the fact that this source is also visible from the southern hemisphere where the Atacama Large Millimeter/submillimeter Array (ALMA), which will be the world’s most advanced sub/millimeter telescope array, is currently 2 under construction in Chile. Observations with ALMA will enable a detailed study of the structure of this galaxy, including the way the gas and dust moves within it.
Dr Richard McMahon, a member of the team from the University of Cambridge in the UK is looking forward to when ALMA is fully operational later this year. “The current observations only provide a glimpse of what ALMA will be capable of when we use it to study the formation of the first generation of galaxies.”
Source: Max-Planck Institute for Astronomy
Image Credits: ESO/UKIDSS/SDSS)
Reference:
B. P. Venemans, R. G. McMahon, F. Walter, R. Decarli, P. Cox, R. Neri, P. Hewett, D. J. Mortlock, C. Simpson, & S. J. Warren (2012). Detection of atomic carbon [CII] 158 micron and dust emission from a
z=7.1 quasar host galaxy APJ Letters arXiv: 1203.5844v1
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