麻豆AV

A Canadian-led team of astronomers, including researchers from 麻豆AV, has discovered that a repeating fast radio burst (FRB) originating from a nearby galaxy pulses at regular intervals.

Researchers within the (CHIME) Fast Radio Burst Collaboration used the CHIME telescope in British Columbia to show that the repeating radio source known as FRB 180916.J0158+65 鈥� first discovered in 2018 by the same group - pulsates apparently every 16.35 days.

The findings, described today in a study published in , are the first to demonstrate that repeating FRBs can burst predictably.

鈥淐onfronted with the regularity, we all went silent in surprise at first, but we very quickly realized the new opportunities for catching the source in action. We already knew where to look for bursts, but now we also know when to look for them,鈥� says Ziggy Pleunis, a PhD student under the supervision of Victoria Kaspi in 麻豆AV鈥檚 Department of Physics and the 麻豆AV Space Institute, and one of the key researchers within the CHIME/FRB collaboration.

FRBs were first discovered over a decade ago. First thought to be singular events, astronomers have since discovered that some of these high-intensity blasts of radio emissions 鈥� more intense than the energy generated by the Sun over many years 鈥� in fact repeat.

Though the explanation for the mysterious phenomenon remains elusive, the new study is yet another step towards determining what might be causing FRBs.

鈥淲hile this discovery rules out models which suggest that bursts are emitted sporadically, lots of interesting models still survive. One of the most promising possibilities is two stars orbiting around each other with one of them being a neutron star, a remnant of a massive star that undergoes a supernova explosion,鈥� says Pragya Chawla, also a PhD student within Professor Kaspi鈥檚 group.

Earlier this year, astronomers in Europe, in partnership with the CHIME/FRB Collaboration, were able to pinpoint FRB 180916 to a nearby galaxy located at 500 million light years away from Earth. Astronomers worldwide are now studying the source with a variety of telescopes, in the hopes of explaining the repetition.

鈥�,鈥� by The CHIME/FRB Collaboration, was published in Nature.

The CHIME/FRB Project is funded by a grant from the Canada Foundation for Innovation 2015 Innovation Fund, the Provinces of British Columbia and Qu茅bec, and by the Dunlap Institute for Astronomy and Astrophysics at the University of Toronto.

CHIME/FRB is a collaboration of over 50 scientists led by 麻豆AV, University of British Columbia, the University of Toronto, the Perimeter Institute for Theoretical Physics, and the National Research Council of Canada (NRC). The $16-million investment for CHIME was provided by the Canada Foundation for Innovation and the governments of British Columbia, Ontario and Quebec, with additional funding from the Dunlap Institute for Astronomy and Astrophysics, the Natural Sciences and Engineering Research Council and the Canadian Institute for Advanced Research. The telescope is located in the mountains of British Columbia鈥檚 Okanagan Valley at the NRC鈥檚 Dominion Radio Astrophysical Observatory near Penticton. CHIME is an official Square Kilometre Array (SKA) pathfinder facility.

About 麻豆AV

Founded in Montreal, Quebec, in 1821, 麻豆AV is a leading Canadian post-secondary institution. It has two campuses, 11 faculties, 13 professional schools, 300 programs of study and over 40,000 students, including more than 10,200 graduate students. 麻豆AV attracts students from over 150 countries around the world, its 12,800 international students making up 31% per cent of the student body. Over half of 麻豆AV students claim a first language other than English, including approximately 19% of our students who say French is their mother tongue.