The stars are surprisingly pure but contain material from an even earlier star, which died in an enormous explosion called hypernova, the researchers said.
"These pristine stars are among the oldest surviving stars in the universe, and certainly the oldest stars we have ever seen," said lead author Louise Howes, a PhD student at the Australian National University (ANU) Research School of Astronomy and Astrophysics.
"These stars formed before the Milky Way, and the galaxy formed around them," said Howes.
"The stars have surprisingly low levels of carbon, iron and other heavy elements, which suggests the first stars might not have exploded as normal supernovae," said Howes.
"Perhaps they ended their lives as hypernovae - poorly understood explosions of probably rapidly rotating stars producing 10 times as much energy as normal supernovae," she said.
Project leader Martin Asplund, professor at ANU Research School of Astronomy and Astrophysics said finding such rare relic stars among the billions of stars in the Milky Way centre was like finding a needle in a haystack.
Following the team's discovery in 2014 of an extremely old star on the edge of the Milky Way, the team focused on the dense central parts of the galaxy, where stars formed even earlier.
The team sifted through about five million stars observed with SkyMapper to select the most pure and therefore oldest specimens, which were then studied in more detail using the Anglo-Australian Telescope in New South Wales and the Magellan telescope in Chile to determine their chemical make-up.
The study was published in the journal Nature.
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