A group of stars hidden in a vast stream of dust and gas that wraps around the Milky Way, which astronomers have been hunting for decades, has been found. These stars could give us clues about the history of two of the Milky Wayâs closest dwarf galaxies, the Large and Small Magellanic Clouds, which feed this ribbon of material.
Up until now, the Magellanic stream, as it is known, appeared to be devoid of stars, despite astronomers predicting that they should exist. That in turn made it hard to measure the streamâs position and velocity.
Now, at Harvard University and his colleagues have identified 13 red giant stars, between 200,000 and 325,000 light years from Earth, that appear to have the same angular momentum and chemical composition as the gas of the Magellanic stream â strongly hinting that they formed from this material.
Advertisement
To make the discovery, the researchers combed through the Gaia catalogue, which contains the positions of and other information on more than a billion stars, filtering out any entries that seem to be moving within the Milky Way. They then further narrowed the field by looking for a group with a similar chemical composition to the Magellanic stream.
âFor the first time we have this stellar counterpart [to the stream], which not only solves this decades-long mystery of why we havenât found [such] stars yet,â says Chandra. âBut it also gives us all of these very useful clues and information about how the gas itself could be moving.â
Knowing more about the stream will also help us understand the Large and Small Magellanic Clouds. Currently, we donât know whether these orbit each other clockwise or anticlockwise, as results from simulations change depending on the position of the Magellanic stream stars. Finding these stars means that we can narrow down more accurate simulations of how the clouds, and the Milky Way, might evolve, says Chandra.
âItâs very exciting,â says at the University of Surrey in the UK. âTheyâre finding this population of stars in the outer galaxy which weâve been searching for for a while.â
However, some of the stars found by Chandra and his team appear to be metal-poor which, unlike the metal-rich stars in the stream, might mean they arenât actually part of it. âThey have shown that those metal-poor stars have similar kinematics to the Magellanic Clouds, so I think I buy their story that itâs connected in some way, but exactly how itâs connected I think is complicated,â says Erkal.
arXiv
