For the first time, an international team of astronomers, led by Dr. James Geach from the University of Hertfordshire, has revealed the dramatic ‘blow out’ phase of galactic evolution.
The astronomers have discovered dense gas being blasted out of a compact galaxy (called SDSS J0905+57) at speeds of up to two million miles per hour. The gas is being driven to distances of tens of thousands of light-years by the intense pressure exerted on it by the radiation of stars that are forming rapidly at the galaxy’s center. This is having a major impact on the evolution of the galaxy.

The team used the Institut de Radioastronomie Millimtrique (IRAM) Plateau de Bure Interferometer, a radio telescope based in the French Alps. By detecting the molecule carbon monoxide, they were able to infer the amount of hydrogen gas present. Stars are born from clouds of hydrogen, so by removing this gas the galaxy can rapidly shut down its star formation. There is enough gas in the outflowing material to form the equivalent of over a billion Suns.

Dr. Geach, who is funded by the Royal Society, explained: “This discovery highlights the serendipity of scientific research. Originally we were simply trying to measure the amount of dense gas in SDSS J0905+57. What we found was something surprising — a large fraction of the gas is being blasted out of the galaxy by the concentration of stars forming at the galaxy’s center.

“We are witnessing the aggressive termination of star formation, and the mechanism by which this is happening is an important new clue in our understanding of the evolution of galaxies.”

Outflows of warm, ionized gas from galaxies are well known, but the team’s observation of large amounts of cold, dense gas being violently removed from the central regions of the galaxy and far into space is a new discovery. Previously it was not known whether the stars alone could drive out gas in this way. Instead, it was thought that energy associated with a growing central black hole would be required, but this is known not to be happening in SDSS J0905+57. This result provides important new insights into how the growth of stars is regulated in galaxies.

Contact:
Kelsey Arif
University of Hertfordshire Press Office
+44 (0)1707 285 163
k.arif3@herts.ac.uk

Reference:
“Stellar feedback as the origin of an extended molecular outflow in a starburst galaxy,” J. E. Geach et al., Nature, 2014 December 4, Volume 516, Issue 7529, Pages 68-70 [http://dx.doi.org/10.1038/nature14012, preprint: http://arxiv.org/abs/1412.1091].

Image caption: This image shows a 3D volume rendering of the IRAM observation of SDSS J0905+57, revealing the detection of carbon monoxide. The bright ‘head’ shows gas associated with the dense, compact star-forming nucleus. The ‘tail’ (color coded in velocity; red=high velocity) shows gas in a high velocity outflow, up to 1,000 km/s, highlighting molecular gas being ejected from the galaxy by stellar feedback. Credit: J. Geach & R. Crain