This cartoon shows how gas falling into distant starburst galaxies ends up in vast turbulent reservoirs of cool gas extending 30 000 light-years from the central regions. ALMA has been used to detect these turbulent reservoirs of cold gas surrounding similar distant starburst galaxies. By detecting CH+ for the first time in the distant Universe, this research opens up a new window of exploration into a critical epoch of star formation.
Credit: ESO/L. Benassi
In the early universe, brilliant starburst galaxies converted vast stores of hydrogen gas into new stars at a furious pace.
Shedding light on this mystery, astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) studied six distant starburst galaxies and discovered that five of them are surrounded by turbulent reservoirs of hydrogen gas, the fuel for future star formation.
These star forming “fuel tanks” were uncovered by the discovery of extensive regions of carbon hydride (CH+) molecules in and around the galaxies. CH+ is an ion of the CH molecule and it traces highly turbulent regions in galaxies that are teeming with hydrogen gas.
The new ALMA observations, led by Edith Falgarone (Ecole Normale Supérieure and Observatoire, Paris, France) and appearing in the journal Nature, help explain how galaxies manage to extend their period of rapid star formation.
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“By detecting these molecules with ALMA, we discovered that there are huge reservoirs of turbulent gas surrounding distant starburst galaxies. These observations provide new insights into the growth of galaxies and how a galaxy’s environs fuel star formation,” said Edwin Bergin, an astronomer with the University of Michigan, Ann Arbor, and co-author on the paper.
“CH+ is a special molecule,” said Martin Zwaan, an astronomer at ESO, who contributed to the paper. “It needs a lot of energy to form and is very reactive, which means its lifetime is very short and it can’t be transported far. CH+ therefore traces how energy flows in the galaxies and their surroundings.”
The observed CH+ reveals dense shock waves, powered by hot, fast galactic winds originating inside the galaxies’ star-forming regions. These winds flow through a galaxy and push material out of it. Their turbulent motions are such that the galaxy’s gravitational pull can recapture part of that material. This material then gathers into turbulent reservoirs of cool, low-density gas, extending more than 30,000 light-years from the galaxy’s star-forming region.
“With CH+, we learn that energy is stored within vast galaxy-sized winds and ends up as turbulent motions in previously unseen reservoirs of cold gas surrounding the galaxy,” said Falgarone. “Our results challenge the theory of galaxy evolution. By driving turbulence in the reservoirs, these galactic winds extend the starburst phase instead of quenching it.”
The team determined that galactic winds alone could not replenish the newly revealed gaseous reservoirs. The researchers suggest that the mass is provided by galactic mergers or accretion from hidden streams of gas, as predicted by current theory.
“This discovery represents a major step forward in our understanding of how the inflow of material is regulated around the most intense starburst galaxies in the early universe,” says ESO’s Director for Science, Rob Ivison, a co-author on the paper. “It shows what can be achieved when scientists from a variety of disciplines come together to exploit the capabilities of one of the world’s most powerful telescopes.”
The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.
Story Source: Materials provided by National Radio Astronomy Observatory Original written by Whitney Clavin.Note: Content may be edited for style and length.
E. Falgarone, M. A. Zwaan, B. Godard, E. Bergin, R. J. Ivison, P. M. Andreani, F. Bournaud, R. S. Bussmann, D. Elbaz, A. Omont, I. Oteo, F. Walter. Large turbulent reservoirs of cold molecular gas around high-redshift starburst galaxies. Nature, 2017; 548 (7668): 430 DOI: 10.1038/nature23298