The first map of the “galactic underworld” — a chart of the corpses of once massive suns that have since collapsed into black holes and neutron stars — has revealed a graveyard that stretches three times the height of the Milky Way and that almost a third of the objects have been flung out from the galaxy altogether. David Sweeney, a Ph.D. student at the Sydney Institute for Astronomy of the University of Sydney and lead author of the paper in the latest issue of Monthly Notices of the Royal Astronomical Society, said:
“These compact remnants of dead stars show a fundamentally different distribution and structure to the visible galaxy. The ‘height’ of the galactic underworld is over three times larger than the Milky Way itself. And an amazing 30 percent of objects have been completely ejected from the galaxy.”
Neutron stars and black holes are formed when massive stars — more than eight times larger than our Sun — exhaust their fuel and suddenly collapse. This triggers a runaway reaction that blows the outer portions of the star apart in a titanic supernova explosion. At the same time, the core keeps compressing itself until it becomes either a neutron star or a black hole, depending on its starting mass. In neutron stars, the core is so dense that electrons and protons are forced to combine at the subatomic level into neutrons, squeezing its total mass into a sphere smaller than a city.
If the original star’s mass exceeds 25 times our Sun’s, that gravity-driven collapse continues until the core is so dense that not even light can escape. Both types of stellar corpses warp space, time, and matter around them. Although billions must have been formed since the galaxy was young, these exotic carcasses were flung out into the darkness of interstellar space by the supernovae that created them, slipping beyond the astronomers’ sight and knowledge. By carefully recreating the entire lifecycle of the ancient dead stars, the researchers have constructed the first detailed map showing where their corpses lie. Sydney Institute for Astronomy’s Professor Peter Tuthill, a co-author of the paper, said:
“One of the problems for finding these ancient objects is that, until now, we had no idea where to look. The oldest neutron stars and black holes were created when the galaxy was younger, shaped differently, and subjected to complex changes spanning billions of years. It has been a major task to model all this to find them.”
Newly-formed neutron stars and black holes conform to today’s galaxy, so astronomers know where to look. But the oldest neutron stars and black holes are like ghosts still haunting a house demolished long ago, so they are harder to find. Professor Tuthill, referring to a place where, according to legend, old elephants go to die alone, far from their group, said:
“It was like trying to find the mythical elephant’s graveyard. The bones of these rare massive stars had to be out there, but they seemed to shroud themselves in mystery.”
Added Sweeney:
“The hardest problem I had to solve in hunting down their true distribution was to account for the ‘kicks’ they receive in the violent moments of their creation. Supernova explosions are asymmetric, and the remnants are ejected at high speed — up to millions of kilometers per hour — and, even worse, this happens in an unknown and random direction for every object.”
But nothing in the universe sits still for long, so even knowing the likely magnitudes of the explosive kicks was not enough. The researchers had to delve into the depths of cosmic time and reconstruct how they behaved over billions of years. Sweeney said:
“It’s a little like in snooker. Knowing which direction the ball is hit and how hard, you can work out where it will end up. But in space, the objects and speeds are just vastly bigger. Plus, the table’s not flat, so the stellar remnants go on complex orbits threading through the galaxy. Finally, unlike a snooker table, there is no friction — so they never slow down. As a result, almost all the remnants ever formed are still out there, sliding like ghosts through interstellar space.”
The Milky Way’s stellar necropolis
The intricate models they built — together with University of Sydney Research Fellow Dr. Sanjib Sharma and Dr. Ryosuke Hirai of Monash University — encoded where the stars were born, met their fiery end, and eventual dispersal as the galaxy evolved. The outcome is a distribution map of the Milky Way’s stellar necropolis. Dr. Sharma said:
“It was a bit of a shock. I work daily with images of the visible galaxy we know today, and I expected that the galactic underworld would be subtly different but similar in broad strokes. I was not expecting such a radical change in form.”
In the maps generated (see images above), the characteristic spiral arms of the Milky Way (top image) have vanished in the “galactic underworld” (lower image). These are entirely washed out because of the age of most of the remnants and the blurring effects of the energetic kicks from the supernovae that created them. Perhaps more surprising, the side-on view shows that the galactic underworld is much more “puffed up” than the Milky Way — a result of kinetic energy injected by supernovae elevating them into a halo around the visible Milky Way. Dr. Hirai said:
“Perhaps the most surprising finding from our study is that the kicks are so strong that the Milky Way will lose some of these remnants entirely. They are kicked so hard that about 30 percent of the neutron stars are flung out into intergalactic space, never to return.”
Added Tuthill:
“For me, one of the coolest things we found in this work is that even the local stellar neighborhood around our Sun is likely to have these ghostly visitors passing through. Statistically, our nearest remnant should be only 65 light years away: more or less in our backyard, in galactic terms.”
Sweeney concluded:
“The most exciting part of this research is still ahead of us. Now that we know where to look, we’re developing technologies to go hunting for them. I’m betting that the galactic underworld won’t stay a mystery for much longer.”
Provided by the University of Sydney [Note: Materials may be edited for content and length.]
