“Oddball Supernova” Appears Strangely Cool Before Exploding – “Stretches What’s Physically Possible!”

Yellow Supergiant in a Close Binary With a Blue, Main Sequence Companion Star

Artist’s impression of a yellow supergiant in a close binary with a blue, main sequence companion star, similar to the properties derived for the 2019yvr progenitor system in Kilpatrick et al. (2021). If the progenitor system to 2019yvr was in such a binary, it must have had a very close interaction that stripped a large amount of hydrogen from the yellow supergiant in the last 100 years before it exploded as a supernova. Credit: Kavli IPMU / Aya Tsuboi

Never-before-seen scenario ‘stretches what’s physically possible.’

A curiously yellow star has caused astrophysicists to reevaluate what’s possible within our universe.

Led by Northwestern University, the international team used NASA’s Hubble Space Telescope to examine the massive star two-and-a-half years before it exploded into a supernova. At the end of their lives, cool, yellow stars are typically shrouded in hydrogen, which conceals the star’s hot, blue interior. But this yellow star, located 35 million lightyears from Earth in the Virgo galaxy cluster, was mysteriously lacking this crucial hydrogen layer at the time of its explosion.

“We haven’t seen this scenario before,” said Northwestern’s Charles Kilpatrick, who led the study. “If a star explodes without hydrogen, it should be extremely blue — really, really hot. It’s almost impossible for a star to be this cool without having hydrogen in its outer layer. We looked at every single stellar model that could explain a star like this, and every single model requires that the star had hydrogen, which, from its supernova, we know it did not. It stretches what’s physically possible.” 

Supernova 2019yvr Explosion Site

Hubble Space Telescope (HST) imaging showing the explosion site of 2019yvr from 2.5 years before its explosion. Upper left: the supernova itself is seen in an image from the Gemini-South telescope 72 days after it exploded. Lower left: a zoom in to the same site in the pre-explosion HST image, showing a single source that appears to be the progenitor star of 2019yvr. Credit: Charles Kilpatrick / Northwestern University

The team describes the peculiar star and its resulting supernova in a new study, which was published on May 5, 2021, in the Monthly Notices of the Royal Astronomical Society. In the paper, the researchers hypothesize that, in the years preceding its death, the star might have shed its hydrogen layer or lost it to a nearby companion star.

Kilpatrick is a postdoctoral fellow at Northwestern’s Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and a member of the Young Supernova Experiment, which uses the Pan-STARSS telescope at Haleakalā, Hawaii, to catch supernovae right after they explode. 

Catching a star before it explodes 

After the Young Supernova Experiment spotted supernova 2019yvr in the relatively nearby spiral galaxy NGC 4666, the team used deep space images captured by NASA’s Hubble Space Telescope, which fortunately already observed this section of the sky. 

“What massive stars do right before they explode is a big unsolved mystery,” Kilpatrick said. “It’s rare to see this kind of star right before it explodes into a supernova.”

The Hubble images showed the source of the supernova, a massive star imaged just a couple of years before the explosion. Although the supernova itself appeared completely normal, its source — or progenitor star — was anything but.

“When it exploded, it seemed like a very normal hydrogen-free supernova,” Kilpatrick said. “There was nothing outstanding about this. But the progenitor star didn’t match what we know about this type of supernova.” 

Direct evidence of violent death

Several months after the explosion, however, Kilpatrick and his team discovered a clue. As ejecta from the star’s final explosion traveled through its environment, it collided with a large mass of hydrogen. This led the team to hypothesize that the progenitor star might have expelled the hydrogen within a few years before its death. 

“Astronomers have suspected that stars undergo violent eruptions or death throes in the years before we see supernovae,” Kilpatrick said. “This star’s discovery provides some of the most direct evidence ever found that stars experience catastrophic eruptions, which cause them to lose mass before an explosion. If the star was having these eruptions, then it likely expelled its hydrogen several decades before it exploded.”

“This star’s discovery provides some of the most direct evidence ever found that stars experience catastrophic eruptions, which cause them to lose mass before an explosion.”
Charles Kilpatrick, astrophysicist

In the new study, Kilpatrick’s team also presents another possibility: A less massive companion star might have stripped away hydrogen from the supernova’s progenitor star. The team, however, will not be able to search for the companion star until after the supernova’s brightness fades, which could take up to 10 years.

“Unlike its normal behavior right after it exploded, the hydrogen interaction revealed it’s kind of this oddball supernova,” Kilpatrick said. “But it’s exceptional that we were able to find its progenitor star in Hubble data. In four or five years, I think we will be able to learn more about what happened.”

For more on this study, read Mysterious Hydrogen-Free Supernova Sheds Light on Massive Stars’ Violent Death Throes.

Reference: “A cool and inflated progenitor candidate for the Type Ib supernova 2019yvr at 2.6 yr before explosion” by Charles D Kilpatrick, Maria R Drout, Katie Auchettl, Georgios Dimitriadis, Ryan J Foley, David O Jones, Lindsay DeMarchi, K Decker French, Christa Gall, Jens Hjorth, Wynn V Jacobson-Galán, Raffaella Margutti, Anthony L Piro, Enrico Ramirez-Ruiz, Armin Rest and César Rojas-Bravo, 30 March 2021, Monthly Notices of the Royal Astronomical Society.
DOI: 10.1093/mnras/stab838

The study, “A cool and inflated progenitor candidate for the type Ib supernova 2019 yvr at 2.6 years before explosion,” was supported by NASA (award numbers GO-15691 and AR-16136), the National Science Foundation (award numbers AST-1909796, AST-1944985), the Canadian Institute for Advanced Research, the VILLUM Foundation and the Australian Research Council Centre of Excellence. In addition to the Hubble Space Telescope, the researchers used instruments at the Gemini Observatory, Keck Observatory, Las Cumbres Observatory, Spitzer Space Telescope and the Swope Telescope.

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