"W49B is the first of its kind to be discovered in the galaxy," said Laura Lopez, who led the study at the Massachusetts Institute of Technology. "It appears its parent star ended its life in a way that most others don't."
Usually when a massive star runs out of fuel, the central region of the star collapses, triggering a chain of events that quickly culminate in a supernova explosion. Most of these explosions are generally symmetrical, with the stellar material blasting away more or less evenly in all directions.
However, in the W49B supernova, material near the poles of the doomed rotating star was ejected at a much higher speed than material emanating from its equator. Jets shooting away from the star's poles mainly shaped the supernova explosion and its aftermath.
"In addition to its unusual signature of elements, W49B also is much more elongated and elliptical than most other remnants," said paper co-author Enrico Ramirez-Ruiz, of the University of California.
"This is seen in X-rays and several other wavelengths and points to an unusual demise for this star."
Most of the time, massive stars that collapse into supernovas leave a dense spinning core called a neutron star. Astronomers can often detect these neutron stars through their X-ray or radio pulses.
However, with W49B, no evidence has been found for a neutron star, implying an even more exotic object might have formed in the explosion, that is, a black hole.
- nzherald.co.nz