Galaxy growth examined like rings of a tree
Scientists have acquired more evidence for the "inside-out" theory of galaxy growth, showing that bursts of star formation in central regions were followed 1 to 2 billion years later by star birth in the outer fringes.
Watching a tree grow might be more frustrating than waiting for a pot to boil, but luckily for biologists, there are tree rings. Beginning at a tree trunk's dense core and moving out to the soft bark, the passage of time is marked by concentric rings, revealing chapters of the tree's history.
Galaxies outlive trees by billions of years, making their growth impossible to see. But like biologists, astronomers can read the rings in a galaxy's disk to unravel its past. Using data from NASA's Wide-field Infrared Survey Explorer (WISE) and Galaxy Evolution Explorer (GALEX), scientists have acquired more evidence for the "inside-out" theory of galaxy growth, showing that bursts of star formation in central regions were followed 1 to 2 billion years later by star birth in the outer fringes.
"Initially, a rapid star-forming period formed the mass at the center of these galaxies, followed later by a star-forming phase in the outer regions. Eventually, the galaxies stop making stars and become quiescent," said Sara Petty of Virginia Tech in Blacksburg, Virginia. "This later star-forming phase could have been caused by minor mergers with gas-rich neighbors, which provide the fuel for new stars."
The discovery also may solve a mystery of elderly galaxies. The galaxies in the study, known as "red and dead" for their red color and lack of new star birth, have a surprising amount of ultraviolet light emanating from the outer regions. Often, ultraviolet light is generated by hot young stars, but these galaxies were considered too old to host such a young population.
The solution to the puzzle is likely hot old stars. Petty and colleagues used a new multiwavelength approach to show that the unexplained ultraviolet light appears to be coming from a late phase in the lives of older stars, when they blow off their outer layers and heat up.
GALEX and WISE turned out to be the ideal duo for the study. GALEX was sensitive to the ultraviolet light, whereas WISE sees the infrared light coming from older stars. GALEX is no longer operating, but WISE was recently reactivated to hunt asteroids, a project called NEOWISE. Both telescopes have large fields of view, allowing them to easily capture images of entire galaxies.
"The synergy between GALEX and WISE produces a very sensitive measurement of where the hot older stars reside in these red-and-dead galaxies," said Don Neill from the California Institute of Technology in Pasadena. "This allows us to map the progress of star formation within each galaxy."