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It is the first time scientists have measured the effect that pulsating, older red stars have on the light of their surrounding galaxy. The findings are published in the Nov. 16 online edition of the journal Nature.
This is an image of the pulsating star T Leporis, compared to the size of the orbit of the Earth around the Sun. T. Leporis is 500 light years away. Huge stars like this are causing the ‘heartbeat’ of the galaxy M87, 50 million light years away.
Credit: ESO/J.-B. Le Bouquin et al.
Until now, no one had considered the effects of these stars on the light coming from more distant galaxies. In distant galaxies the light of each pulsating star is mixed with the light of many more stars that do not vary in brightness.
“We realized that these stars are so bright and their pulsations so strong that they are difficult to hide,” said Charlie Conroy, an assistant professor at Harvard, who led the research. “We decided to see if the pulsations of these stars could be detected even if we could not separate their light from the sea of unchanging stars that are their neighbors.”
The researchers used a unique series of images of the galaxy M87, in the constellation Virgo, taken with the Hubble Space Telescope over the course of three months in 2006. They quickly found what they were looking for: 25% of the pixels in the Hubble image of M87 go up and down in brightness, as if the galaxy had a heartbeat. The mean pulse of the stars in M87 is about one beat every 270 days.
The next step, according to the researchers, is to take the pulse of other galaxies. “Our models suggest that the pulsations will be stronger in younger galaxies, and that’s something we’d love to test,” said co-author Jieun Choi, a Harvard graduate student.
Of course, even the older galaxies will continue to beat for a while longer. “Cardiac arrest is not expected until a trillion years from now,” van Dokkum said. “That’s a hundred times longer than the age of the universe.”
Jim Shelton
Yale University