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Posted: Apr 25, 2013
Entire galaxies feel the heat from newborn stars
(Nanowerk News) When galaxies form new stars, they sometimes do so in frantic episodes of activity known as starbursts. These events were commonplace in the early Universe, but are rarer in nearby galaxies.
During these bursts, hundreds of millions of stars are born, and their combined effect can drive a powerful wind that travels out of the galaxy. These winds were known to affect their host galaxy -- but this new research now shows that they have a significantly greater effect than previously thought.
An international team of astronomers observed 20 nearby galaxies, some of which were known to be undergoing a starburst. They found that the winds accompanying these star formation processes were capable of ionising  gas up to 650 000 light-years from the galactic centre -- around twenty times further out than the visible size of the galaxy. This is the first direct observational evidence of local starbursts impacting the bulk of the gas around their host galaxy, and has important consequences for how that galaxy continues to evolve and form stars.
This illustration shows a messy, chaotic galaxy undergoing bursts of star formation. This star formation is intense; it was known that it affects its host galaxy, but this new research shows it has an even greater effect than first thought. The winds created by these star formation processes stream out of the galaxy, ionising gas at distances of up to 650 000 light-years from the galactic center. (Credit: ESA, NASA, L. Calçada)
"The extended material around galaxies is hard to study, as it's so faint," says team member Vivienne Wild of the University of St. Andrews. "But it's important -- these envelopes of cool gas hold vital clues about how galaxies grow, process mass and energy, and finally die. We're exploring a new frontier in galaxy evolution!"
The team used the Cosmic Origins Spectrograph (COS) instrument  on the NASA/ESA Hubble Space Telescope to analyse light from a mixed sample of starburst and control galaxies. They were able to probe these faint envelopes by exploiting even more distant objects -- quasars, the intensely luminous centres of distant galaxies powered by huge black holes. By analysing the light from these quasars after it passed through the foreground galaxies, the team could probe the galaxies themselves.
"Hubble is the only observatory that can carry out the observations necessary for a study like this," says lead author Sanchayeeta Borthakur, of Johns Hopkins University. "We needed a space-based telescope to probe the hot gas, and the only instrument capable of measuring the extended envelopes of galaxies is COS."
The starburst galaxies within the sample were seen to have large amounts of highly ionised gas in their halos -- but the galaxies that were not undergoing a starburst did not. The team found that this ionisation was caused by the energetic winds created alongside newly forming stars.
This has consequences for the future of the galaxies hosting the starbursts. Galaxies grow by accreting gas from the space surrounding them, and converting this gas into stars. As these winds ionise the future fuel reservoir of gas in the galaxy's envelope, the availability of cool gas falls -- regulating any future star formation.
"Starbursts are important phenomena -- they not only dictate the future evolution of a single galaxy, but also influence the cycle of matter and energy in the Universe as a whole," says team member Timothy Heckman, of Johns Hopkins University. "The envelopes of galaxies are the interface between galaxies and the rest of the Universe -- and we're just beginning to fully explore the processes at work within them."
The team's results will appear in the 1 May 2013 issue of The Astrophysical Journal.
 A gas is said to be ionised when its atoms have lost one or more electrons -- in this case by energetic winds exciting galactic gas and knocking electrons out of the atoms within.
 Spectrographs are instruments that break light into its constituent colours and measure the intensity of each colour, revealing information about the object emitting the light -- such as its chemical composition, temperature, density, or velocity.