U. MICHIGAN (US) — Old galaxies long thought to be finished making stars are still alive and producing at low levels, according to new research.
Using the Wide Field Camera 3 on the Hubble Space Telescope, researchers saw individual young stars and star clusters in four galaxies that are about 40 million light years away. One light year is about 5.9 trillion miles.
Galaxies generally come in two types: spiral galaxies, like the Milky Way, and elliptical galaxies. The stars in spiral galaxies lie in a disk that also contains cold, dense gas from which new stars are regularly formed at a rate of about one sun per year.
Stars in elliptical galaxies, on the other hand, are nearly all billions of years old. These galaxies contain stars that orbit every which way, like bees around a beehive. Ellipticals have little, if any, cold gas, and no star formation was previously known.
“Astronomers previously studied star formation by looking at all of the light from an elliptical galaxy at once, because we usually can’t see individual stars,” says Alyson Ford, research fellow at the University of Michigan. “Our trick is to make sensitive ultraviolet images with the Hubble Space Telescope, which allows us to see individual stars.”
The technique enabled the astronomers to observe star formation, even if it is as little as one sun every 100,000 years.
Ford and Joel Bregman, professor of astronomy, are studying the stellar birth rate and likelihood of stars forming in groups within ellipticals.
In the Milky Way, stars usually form in associations containing from tens to 100,000 stars. In elliptical galaxies, conditions are different because there is no disk of cold material to form stars.
“We were confused by some of the colors of objects in our images until we realized that they must be star clusters, so most of the star formation happens in associations,” Ford says.
The team’s breakthrough came when they observed Messier 105, a normal elliptical galaxy 34 million light years away in the constellation Leo. Though there had been no previous indication of star formation in Messier 105, Ford and Bregman saw a few bright, very blue stars, resembling a single star 10 to 20 times the mass of the sun.
They also saw objects that aren’t blue enough to be single stars, but instead are clusters of many stars. Accounting for these clusters, stars are forming in Messier 105 at an average rate of one sun every 10,000 years. “This is not just a burst of star formation but a continuous process,” Ford says.
The findings raise new mysteries, such as the origin of the gas that forms the stars. “We’re at the beginning of a new line of research, which is very exciting, but at times confusing,” Bregman says.
“We hope to follow up this discovery with new observations that will really give us insight into the process of star formation in these ‘dead’ galaxies.”
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