The object, a white dwarf designated RXJ0528+2838 located 730 light-years from Earth, was captured by the VLT that showed the presence of a massive bow shock of glowing material similar to the wake created by a ship moving through water. Typically, such structures are powered by intense outflows of gas and dust from active, living stars. However, RXJ0528+2838 is a dead stellar remnant that shouldhave long since exhausted its nuclear fuel. Like other white dwarfs, it's expected to be a quiet, slowly cooling relic.
European Southern Observatory’s Very Large Telescope
The shock wave isn't just a structural anomaly either. When viewed through the VLT’s MUSE instrument, the shock wave shimmers with a multi-hued glow. These colors represent specific chemical signatures, with red, green, and blue hues indicating the presence of hydrogen, nitrogen, and oxygen (respectively) being energized as the star moves through space. This bow wave stretches roughly 3,800 times the distance between the Earth and the Sun, suggesting an energetic process that has been active for at least 1,000 years.
Current astrophysical models suggest that for a white dwarf to produce this kind of outflow, it must first siphon material from a companion star into a spinning accretion disk, which then acts as a launchpad for the gas. Yet, RXJ0528+2838 shows absolutely no evidence of such a disk, even though it has a low-mass companion star. Astronomers believe RXJ0528+2838’s exceptionally strong magnetic field might be the culprit, acting as a "mystery engine" that channels stolen material directly onto the star's surface. However, even this theory hits a snag: standard data suggests the magnetic field is only strong enough to power a shock wave for a few hundred years, not the millennium-long duration observed.
"We found something never seen before and, more importantly, entirely unexpected," said Scaringi.
This energy leak from a supposedly quiet star challenges fundamental assumptions about how binary stars evolve and interact with the interstellar medium. Perhaps this unique, glowing contradiction of a star foretells how big of a role extreme magnetic environments play in something supposedly inactive.
Main image: Highlighted square shows shock waves around the dead star RXJ0528+2838. (Credit: ESO/K. Ilkiewicz and S. Scaringi et al. Background: PanSTARRS)