Evidence found of white dwarf remnant after supernova
by Bob Yirka , Phys.org
Image of the accretion disk: A snapshot of the binary star system before the violent supernova explosion blew it to pieces. Credit: Copyright Russell Kightley
An international team of space scientists has found evidence of what they believe is a remnant of a type Iax supernova—a white dwarf moving in a way that suggests it was blown across part of the universe by the power of a thermonuclear explosion. In their paper published in the journal Science, the team describes their study of the star and why they believe it is the remains of an Iax supernova.
Most space scientists agree that supernovae occur when a white dwarf pulls a certain amount of the outer layer from a nearby star until it reaches a tipping point—when that happens, a thermonuclear explosion occurs, obliterating the white dwarf—at least, most of the time. This so-called normal type of supernova is classified as Ia. But some theories suggest that the explosion is sometimes not strong enough to completely obliterate the white dwarf—some of it is left behind and pushed through space at a very high speed due to the energy of the explosion. Such supernovae are labeled Iax, but until now, none had ever actually been observed. In this new effort, the research team describes a white dwarf that appears to have all the markings of a supernova Iax remnant.
The star, called LP 40-365, was actually first spotted back in 2013—it drew attention because it was traveling so fast. The researchers found that the star was spinning faster than expected and that it had a mixed composition, which suggested that it very likely once had a companion star.
The progenitor of LP40-365 could be a binary star system like the one shown in this animation. Here, an ultra-massive and compact dead star called a white dwarf (shown as a small white star) is accreting matter from its giant companion (the larger red star). The material escapes from the giant and forms an accretion disk around the white dwarf. Once enough material is accreted onto the white dwarf, a violent thermonuclear runaway tears it apart and destroys the entire system. The giant star and the surviving fragment of the white dwarf are flung into space at tremendous speeds. The surviving white dwarf shrapnel hurtles towards our region of the Galaxy, where its radiation is detected by ground based telescopes. Credit: Copyright Russell Kightley
The researchers also note that in most cases, stars that move faster than normal are doing so because they were flung across their galaxy after traveling too close to its center. But the trajectory of LP 40-365 showed that it had not approached the center of its galaxy.
The team suggests the evidence indicates that the white dwarf is most likely the remnant of a supernova—one that occurred between 5 and 50 million years ago. The team and likely others will continue to study the star to add further proof to their assumption. They believe it will help in better understanding what happens prior to a supernova, regardless of type.
00.0sec: Initial binary star outside the disk of the Milky Way galaxy. A massive white dwarf accreting material through an accretion disk from its red giant companion star. The stars orbit around the center of mass of the binary system. 14.6sec: The white dwarf reaches the Chandrasekhar mass limit and explodes as a bright Type Ia supernova. However, the explosion is not perfect; a fraction of the white dwarf shoots out like a shrapnel to the left. The binary system disrupts. 18.0sec: The supernova explosion again, at an edge-on view. The shrapnel comes at the viewer and passes by. 20.0sec: After passing by, the remnant flies off towards the disk of the Milky Way towards the spiral arm with the Solar System. 24.0sec: The fast moving remnant from the solar neighborhood as it passes by the stars in our galactic arm, including the Sun. The remnant gets in the reach of our telescopes. Credit: Copyright Sardonicus Pax
More information:
S. Vennes et al. An unusual white dwarf star may be a surviving remnant of a subluminous Type Ia supernova, Science (2017). DOI: 10.1126/science.aam8378
Citation:
Evidence found of white dwarf remnant after supernova (2017, August 18)
retrieved 25 May 2022
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Evidence found of white dwarf remnant after supernova
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