We've got the beat: Astronomers discover a distant galaxy with a pulse

We've got the beat: Astronomers discover a distant galaxy with a pulse
Hubble Space Telescope photograph of the galaxy M87, which is 50 million light years from Earth. Credit: NASA/ESA

Astronomers at Yale and Harvard have found a galaxy with a heartbeat—and they've taken its pulse.

It is the first time scientists have measured the effect that pulsating, older red have on the light of their surrounding galaxy. The findings are published in the Nov. 16 of the journal Nature.

"We tend to think of galaxies as steady beacons in the sky, but they are actually 'shimmering' due to all the giant, pulsating stars in them," said Pieter van Dokkum, the Sol Goldman Professor and chair of astronomy at Yale, and co-author of the study.

Later in life, stars like our Sun undergo significant changes. They become very bright and swell up to an enormous size, swallowing any planets within a radius roughly equivalent to Earth's distance from the Sun. Near the end of their lifetime, they begin to pulsate, increasing and decreasing their brightness every few hundred days. In our Milky Way galaxy, many stars are known to be in this phase.

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."

We've got the beat: Astronomers discover a distant galaxy with a pulse
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.

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.

Discovery measures 'heartbeats' of distant galaxy's stars
The monstrous elliptical galaxy M87, located 53 million light-years from Earth is the dominant galaxy at the center of the neighboring Virgo cluster of galaxies. Astronomers have measured the 'heartbeats' of stars within M87 and used that data to determine the galaxy's age in a new way. This photograph was taken with the Hubble Space Telescope's Advanced Camera for Surveys instrument. Credit: NASA, ESA, and the Hubble Heritage Team

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."


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More information: Ubiquitous time variability of integrated stellar populations, Nature, DOI: 10.1038/nature15731
Journal information: Nature

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Citation: We've got the beat: Astronomers discover a distant galaxy with a pulse (2015, November 16) retrieved 18 April 2019 from https://phys.org/news/2015-11-weve-astronomers-distant-galaxy-pulse.html
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Nov 16, 2015
Why is there a coherent pulse at all? My expectation is that if the individual stellar pulses are not actually synced to one another through some mechanism, then this should be noise.

Nov 16, 2015
Why is there a coherent pulse at all? My expectation is that if the individual stellar pulses are not actually synced to one another through some mechanism, then this should be noise.


And your paper showing these resuls? Is where? More pseudocr*p, ladies and gentlemen.

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