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| An image of the binary stars Alpha Centauri A (left) and Alpha Centauri B, taken by the Hubble Space Telescope. Image Credit: NASA |
When supermassive stars are born, they’re almost always paired with a twin, and the two stars normally orbit one another.
But astronomers at UCLA’s Galactic Center Group and the Keck Observatory have analyzed over a decade’s worth of data about 16 young supermassive stars orbiting the supermassive black hole at the center of the Milky Way galaxy. Their findings, published today in the Astrophysical Journal, reveal a startling conclusion: All of them are singletons.
But why? Are the stars, which are about 10 times larger than our sun, being formed alone in the hostile environment around the black hole? Have their “twins” been kicked out by the black hole? Or have pairs of stars merged to form single stars?
The findings support a scenario in which the central supermassive black hole drives nearby stellar binaries to merge or be disrupted, with one of the pair being ejected from the system.
The stars the scientists observed are known as S-stars, and most of them are young — formed within the past 6 million years — and massive. They are mostly located within a light-month, or a little under 500 billion miles, of the black hole.
“Stars this young shouldn’t even be near the black hole in the first place,” said UCLA postdoctoral scholar Devin Chu, the study’s first author. “They couldn’t have migrated to this region in just 6 million years. But to have a star form in such a hostile environment is surprising.”
Chu and his colleagues used data taken with Keck’s adaptive optics instruments to conduct the first-ever search for spectroscopic binary stars among the S-stars. Spectroscopic binary stars appear through optical telescopes to be single stars but, when the light they emit is analyzed by scientists, are revealed to actually be pairs of stars.
All of the S-stars that appeared to be single were, in fact, alone.
Even more surprising, the researchers found that the number of pairs of S-stars that could possibly exist near the black hole was much lower than the number of comparable stars in the section of space surrounding Earth’s sun, known as the solar neighborhood.
They did this by calculating a metric called the binary fraction, which defines how many stars in a given area could come in pairs; the higher the binary fraction, the more stars that could exist in pairs. Previous studies have shown that the binary fraction for stars similar to S-stars in Earth’s solar neighborhood is around 70%. In the new study, the researchers found that near the Milky Way’s black hole, the upper limit is just 47% —suggesting that the extreme environment of the black hole is limiting the survival of stellar binaries.
“This difference speaks to the incredibly interesting environment of the center of our galaxy; we’re not dealing with a normal environment here,” Chu said. “This also suggests that the black hole drives these nearby binary stars to merge or be disrupted, which has important implications for the production of gravitational waves and hypervelocity stars ejected from the galactic center.”
The UCLA researchers now plan to explore how the limit on the binary fraction they calculated compares to the binary fraction for similar stars that are located farther from the black hole, but still within its gravitational influence.
Published in journal: Astrophysical Journal
Source/Credit: University of California, Los Angeles | Holly Ober
Reference Number: astr051123_03
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