The Milky Way globular cluster Omega Centauri contains stars that are currently estimated to be between 10 billion and 12 billion years old.
ESO/INAF-VST/OmegaCAM; Acknowledgement: A. Grado, L. Limatola/INAF-Capodimonte Observatory
Globular clusters are spherical associations of old stars, thought to have formed during the earliest days of our universe, nearly 14 billion years ago. They contain some of the oldest stars in our galaxy, and the same appears true for other galaxies as well. But new research led by astronomers at the University of Warwick is now challenging this belief, showing that globular clusters may be a full 4 billion years younger than previously thought. Published May 24 in Monthly Notices of the Royal Astronomical Society, the paper states that globular clusters may be closer to 9 billion years in age than the previously measured value of 13 billion years.
How did this age discrepancy arise? The age of globular clusters has long been determined by studying the light from their stars. Astronomers compare the properties of the integrated (total) light received from globular clusters with templates of starlight produced by stars of different ages and types. (It’s worth noting that at one point, these models showed that globular clusters were older than the universe, so this wouldn’t be the first time astronomers have updated their age estimates for these objects.)
This new study takes a different approach, using new models called Binary Population and Spectral Synthesis (BPASS) models, which take into account the effects of binary stars and how the evolution of binary systems — which are known to be common — affects the light received from globular clusters. The idea is this: interactions between binary stars can change the properties of the starlight emitted by one star as elements from its atmosphere are stripped away by the gravity of a companion. When taken into account these binary interactions could make the starlight coming from globular clusters look more like the older templates used by astronomers to determine stellar age, prematurely aging the cluster.
How did this age discrepancy arise? The age of globular clusters has long been determined by studying the light from their stars. Astronomers compare the properties of the integrated (total) light received from globular clusters with templates of starlight produced by stars of different ages and types. (It’s worth noting that at one point, these models showed that globular clusters were older than the universe, so this wouldn’t be the first time astronomers have updated their age estimates for these objects.)
This new study takes a different approach, using new models called Binary Population and Spectral Synthesis (BPASS) models, which take into account the effects of binary stars and how the evolution of binary systems — which are known to be common — affects the light received from globular clusters. The idea is this: interactions between binary stars can change the properties of the starlight emitted by one star as elements from its atmosphere are stripped away by the gravity of a companion. When taken into account these binary interactions could make the starlight coming from globular clusters look more like the older templates used by astronomers to determine stellar age, prematurely aging the cluster.
Stars in binary systems could be affected by interactions with their companions. Here, one star strips material from another, affecting the light it emits.
Mark A. Garlick/University of Warwick
“Determining ages for stars has always depended on comparing observations to the models which encapsulate our understanding of how stars form and evolve,” said lead author Elizabeth Stanway of the University of Warwick’s Astronomy and Astrophysics Group in a press release. “That understanding has changed over time, and we have been increasingly aware of the effects of stellar multiplicity — the interactions between stars and their binary and tertiary companions.”
BPASS models have previously been used to successfully determine the age of young stellar populations, both within the Milky Way and in extremely distant galaxies, but even with this age revision, globular clusters are still old. The next step, Stanway said, is to look at nearby globular clusters in which individual stars can be seen (faraway clusters just look like fuzzy balls, so all astronomers have to work with is the total light from all their stars together). Studying nearby clusters in better detail and comparing these results with the BPASS models should bring to light the accuracy of the models and this new age measurement.
But “If true,” she said, “it changes our picture of the early stages of galaxy evolution and where the stars that have ended up in today’s massive galaxies, such as the Milky Way, may have formed.”
BPASS models have previously been used to successfully determine the age of young stellar populations, both within the Milky Way and in extremely distant galaxies, but even with this age revision, globular clusters are still old. The next step, Stanway said, is to look at nearby globular clusters in which individual stars can be seen (faraway clusters just look like fuzzy balls, so all astronomers have to work with is the total light from all their stars together). Studying nearby clusters in better detail and comparing these results with the BPASS models should bring to light the accuracy of the models and this new age measurement.
But “If true,” she said, “it changes our picture of the early stages of galaxy evolution and where the stars that have ended up in today’s massive galaxies, such as the Milky Way, may have formed.”