Three runaway stars believed to be survivors of thermonuclear explosions

stars
Credit: CC0 Public Domain

A team of researchers with members from Germany, the U.K. and the U.S. has found what they describe as three stars that are example remnants of thermonuclear explosions. They have written a paper describing their findings and have uploaded it to the arXiv preprint server and onto Oxford's Monthly Notices of the Royal Academic Astronomical Society.

One of the ways a supernova occurs is when a white dwarf runs out of fuel. As fuel begins to run low, hydrogen in the interior shrinks, and pressure and heat increase, causing large elements to fuse together. As the balance of gravity and inner pressure become out of tune, the star begins to collapse and a thermonuclear occurs, bursting through the star's outer layers. Following the supernova, what is left of the star forms either a neutron star or a black hole. In this new effort, the researchers report finding evidence of a different outcome—a partially burnt stellar remnant.

Prior research has suggested that when some white dwarf stars explode, they do so with less intensity than others—they are known as "type lax" explosions. And because they are less intense, the star actually survives the blast, albeit with lower mass. Theory suggests that such stars would be pushed across the universe by the force of the blast. Some have suggested that the low-mass white dwarf LP 40-365 is an example of such a star. In this new effort, the researchers report finding three more stars that seem to fit the new category of white dwarf.

While studying data from ESA's Gai space telescope, the researchers found the three stars, which stood out because they were all smaller than is the norm for a white dwarf. And they all had unique trajectories. Two of the stars were moving at very high speed across the Milky Way on a path that will take them out of the galaxy altogether. The third was found to be traveling in the opposite direction of the other stars in the galaxy. The researchers suggest their findings indicate that it is time to name a new class of white dwarf for those that survive explosion. They also note that future study of such stars could lead to a better understanding of the conditions that lead to exploding.


Explore further

Evidence found of white dwarf remnant after supernova

More information: R Raddi et al. Partly burnt runaway stellar remnants from peculiar thermonuclear supernovae, Monthly Notices of the Royal Astronomical Society (2019). DOI: 10.1093/mnras/stz1618

arxiv.org/abs/1902.05061

© 2019 Science X Network

Citation: Three runaway stars believed to be survivors of thermonuclear explosions (2019, July 8) retrieved 21 July 2019 from https://phys.org/news/2019-07-runaway-stars-believed-survivors-thermonuclear.html
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.
825 shares

Feedback to editors

User comments

Jul 08, 2019
I know the odds are against it, but imagine if that star moving against the spin of the galaxy actually hits another star. That is a video I wouldn't mind watching.

Jul 09, 2019
This article is greatly simplified, a requirement.
Another simple equation accepted for a great many years concerns gravitational collapse. Any irregularities shrink with the collapse, resulting in a more and more perfect sphere as it shrinks. Without this factor black holes become much more difficult to form.

On the face of it these new findings seem a contradiction. We shall see.

Jul 09, 2019
Jeffhans1, apparently, with their detection of two neutron stars colliding, it was similar to what you are wanting to see. They had the gravity wave detection from it, and then also an extreme brightening of the area that grew much brighter, for a wider area than had been estimated, and now we (think) we understand that the afterglow was from thrown off neutron material degenerating back to proton and electron masses of such heavy mass as to be highly radioactive, with several short half-live isotopes degrading rapidly and later, once it got down to the longer half-life materials, the light started dimming back down.

So we almost have a picture of that sort of thing happening a long time ago, in a galaxy far, far away...

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more