UW News

Melissa Graham

January 10, 2019

Astronomers find signatures of a ‘messy’ star that made its companion go supernova

An image of a galaxy in outer space, with a bright supernova visible at its outer edge.

On Jan. 10 at the 2019 American Astronomical Society meeting in Seattle, an international team of astronomers announced that they have identified the type of companion star that made its partner in a binary system, a carbon-oxygen white dwarf star, explode. Through repeated observations of SN 2015cp, a supernova 545 million light years away, the team detected hydrogen-rich debris that the companion star had shed prior to the explosion.