“The rest of the galaxy is done maturing,” said Kartik Sheth of the National Radio Astronomy Observatory of Charlottesville, Virginia. “But the outer ring is just now starting to light up with stars.”
NGC 1291 is located about 33 million light-years away in the constellation Eridanus. It is what’s known as a barred galaxy because its central region is dominated by a long bar of stars. (In the new image, the bar is within the blue circle and looks like the letter S.)
The bar formed early in the history of the galaxy. It churns material around, forcing stars and gas from their original circular orbits into large noncircular, radial orbits. This creates resonances — areas where gas is compressed and triggered to form new stars. Our Milky Way Galaxy has a bar, though not as prominent as the one in NGC 1291.
Sheth and his colleagues are busy trying to better understand how bars of stars like these shape the destinies of galaxies. In a program called Spitzer Survey of Stellar Structure in Galaxies, Sheth and his team of scientists are analyzing the structures of more than 3,000 galaxies in our local neighborhood. The farthest galaxy of the bunch lies about 120 million light-years away — practically a stone’s throw in comparison to the vastness of space.
The astronomers are documenting structural features, including bars. They want to know how many of the local galaxies have bars, as well as the environmental conditions in a galaxy that might influence the formation and structure of bars.
“Now, with Spitzer, we can measure the precise shape and distribution of matter within the bar structures,” said Sheth. “The bars are a natural product of cosmic evolution, and they are part of the galaxies’ endoskeleton. Examining this endoskeleton for the fossilized clues to their past gives us a unique view of their evolution.”
In the Spitzer image, shorter-wavelength infrared light has been assigned the color blue, and longer-wavelength light, red. The stars that appear blue in the central bulge region of the galaxy are older; most of the gas, or star-making fuel, there was previously used up by earlier generations of stars. When galaxies are young and gas-rich, stellar bars drive gas toward the center, feeding star formation.
Over time, as the fuel runs out, the central regions become quiescent and star-formation activity shifts to the outskirts of a galaxy. There, spiral density waves and resonances induced by the central bar help convert gas to stars. The outer ring, seen here in red, is one such resonance area where gas has been trapped and ignited into star-forming frenzy.
