The findings appear in a paper in the Jan,
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. 5 Nature and two papers in the Jan,
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. 10 Astrophysical Journal Letters.
“Without a doubt, this is a landmark event,
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,” said Duncan Lorimer, an astrophysicist at West Virginia University who was not involved with these studies but did discover the first radio burst roughly a decade ago. “There’s no question about the validity of the result.”
The host galaxy is tiny. “We’re barely able to distinguish it from a star,” said project member Shriharsh Tendulkar,
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, an astrophysicist at McGill University in Montreal. It has roughly one one-thousandth of the stars as the Milky Way and is less than one-tenth as wide. “That’s weird,
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,” he said. One favored explanation for fast radio bursts is that they come from neutron stars,
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, the dense cores left behind after a massive star explodes. But if neutron stars are responsible,
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, then astronomers expect to find bursts in places with lots of stars, Tendulkar said.
Tracing FRB 121102 back to a dwarf galaxy doesn’t rule out neutron stars as a source. The gas in dwarf galaxies is more pristine than in other locales such as the Milky Way — with relatively low amounts of elements heavier than helium. Such gas makes it easier for massive stars to form. More heavyweight stars lead to more neutron stars,
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, which could lead to more radio bursts.

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