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Astronomers discover the Ed Begley Jr. of galaxies

An international team of researchers have spotted the most fuel-efficient galaxy yet, which converts nearly 100 percent of its hydrogen gas into stars.


The tiny red spot in this image is one of the most efficient star-making galaxies ever observed, converting gas into stars at the maximum possible rate. Visible-light observations from NASA's Hubble Space Telescope (inset) reveal that the starlight in this galaxy is extraordinarily compact, with most of the light emitted by a region just a fraction of the size of the Milky Way galaxy.


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Six billion or so light years from here, there's a galaxy that seems to take seriously the old Lakota maxim about using the whole buffalo.

Except by "use" we mean "form stars out of" and by "buffalo" we mean "interstellar hydrogen gas." 

Hydrogen gas is the fuel that galaxies use to make new stars, and most galaxies are the equivalent of a Hummer with a broken oxygen sensor, four flat tires, and a buffalo carcass strapped to the roof. Most of the gas meant to transport you gets wasted. But a new study has spotted a galaxy that is converting gas into stars at a rate hundreds of times that of our galaxy with almost 100 percent efficiency.

An international team of scientists looked at data from NASA's Wide-field Infrared Survey Explorer (WISE) and spotted a galaxy that was just blazing with infrared radiation, equivalent, they say, to a trillion suns. Observations from the Hubble telescope confirmed that the galaxy, which is affectionately known as SDSSJ1506+54, is extremely compact, with most of the infrared light pouring from an area that is a fraction of the size of our own Milky Way. 

The researchers then used data from the IRAM Plateau de Bure interferometer in the French Alps to detect the presence of carbon monoxide, which indicates the presence of hydrogen. By combining the gas measurements with the rate of star formation, the scientists found that the galaxy was forming stars out of the gas at a rate that is close to the theoretical maximum. Their paper, which has been accepted for publication in the Journal of Astrophysical Letters, calls it "star formation at its most extreme."


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