‘Missing fuel’ for star formation identified
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Last Updated: Friday, August 26, 2011, 16:31
  
Washington: A new study by Nicolas Lehner and Christopher Howk, faculty in the Department of Physics at the University of Notre Dame has indicated that the Milky Way will have the fuel to continue forming stars, thanks to massive clouds of ionized gas raining down from its halo and intergalactic space.

Using the Cosmic Origins Spectrograph, one of the newest instruments on the NASA/ESA Hubble Space Telescope, the researchers measured for the first time the distances to fast-moving clouds of ionized gas previously seen covering a large fraction of the sky. These fast-moving clouds reside in the distant reaches of the Milky Way and contain huge quantities of gas.

The Milky Way would rapidly change its gas into stars if no supply of new matter were available to replenish the gas. Astronomers have hypothesized that the ionized fast-moving gas clouds could be this reservoir of gas, but it was not known if they were interacting with the Milky Way.

“Our findings explain why the Milky Way can keep having star formation,” said Lehner.

“Knowing the distances to these clouds tells us where the gaseous fuel is for forming stars over billions of years,” added Lehar.

Gas clouds can be identified and studied because elements in the cloud absorb small amounts of the light from a star or other light source as it passes through a cloud on its way to the Earth. The characteristic “fingerprint” left in the spectrum allows astronomers to determine the properties of the gas.

Lehner and Howk identified 27 stars around the Milky Way, whose distances were known, and used the Hubble to take line-of-sight readings of light coming from them.

Results from the stellar sample showed the ionized clouds largely resided in the Milky Way’s halo. The authors concluded that these flows of ionized gas are within about one Galactic radius (40,000 light-years) of Earth. The new Hubble observations revealed the presence of ionized gas in half the stellar sample, comparable to the fraction observed toward more distant quasars.

“We know now where is the missing fuel for Galactic star formation,” said Lehner.

“We now have to learn how it got there,” he added.

The study appears in Science.

ANI


First Published: Friday, August 26, 2011, 16:31


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