1 minute read

SUPERNOVA ORIGIN REVEALED BY RADIO SIGNAL

Next Article
Science Quiz

Science Quiz

before the white dwarf's explosion, according to the recent finding of supernova SN 2020eyj.

Erik Kool, post-doc at the Department of Astronomy at Stockholm University and the paper's primary author, adds, "Once we saw the signatures of strong interaction with the material from the companion, we tried to also detect it in radio emission." Astronomers have been attempting to find a Type Ia supernova for decades, but this is the first radio discovery of one.

Advertisement

Astronomers from Stockholm University describe the origin of a thermonuclear supernova explosion in the most recent edition of the journal Nature The exploding white dwarf star had a helium-rich companion, as evidenced by the strong helium emission lines and the first observation of such a supernova in radio waves.

Astronomers value Type Ia supernova because they can use them to gauge the universe's expansion The cause of these explosions, however, is yet unknown. The precise mechanism and the make-up of the progenitor are unknown, but it is known that the explosion is caused by a compact white dwarf star accreting too much matter from a partner star The companion star was a helium star that had lost a lot of its material soon

Supernova 2020eyj was discovered by the Zwicky Transient Facility camera on Palomar mountain, where the Oskar Klein Centre at Stockholm University is members. "The Nordic Optical telescope on La Palma was fundamental for following up this supernova", says Professor Jesper Sollerman at the Department of Astronomy and co-author of the paper "As were spectra from the large Keck telescope on Hawai'i that immediately revealed the very unusual helium-dominated material around the exploded star."

"This is clearly a very unusual Type Ia supernova, but still related to the ones we use to measure the expansion of the universe", adds Joel Johansson from the Department of Physics. "While normal Type Ia supernova appear to always explode with the same brightness, this supernova tells us that there are many different pathways to a white dwarf star explosion", he adds.

This article is from: