Planetary nebulae are shells of gas and dust expelled by stars near the end of their lives and are typically seen around stars comparable or smaller in size than the Sun.
The international team, led by Associate Professor Miroslav Filipovic from the University of Western Sydney, surveyed the Magellanic Clouds, the two companion galaxies to the Milky Way, with radio telescopes of the Commonwealth Scientific and Industrial Research Organisation (CSIRO) Australia Telescope National Facility.
They noticed that 15 radio objects in the Clouds match with well-known planetary nebulae observed by optical telescopes.
The new class of objects are unusually strong radio sources.
Whereas the existing population of planetary nebulae is found around small stars comparable in size to our Sun, the new population may be the long predicted class of similar shells around heavier stars.
Filipovic's team argues that the detections of these new objects may help to solve the so called "missing mass problem" - the absence of planetary nebulae around central stars that were originally 1 to 8 times the mass of the Sun.
Up to now most known planetary nebulae have central stars and surrounding nebulae with respectively only about 0.6 and 0.3 times the mass of the Sun but none have been detected around more massive stars.
The new Super Planetary Nebulae are associated with larger original stars (progenitors), up to 8 times the mass of the Sun. And the nebular material around each star may have as much as 2.6 times the mass of the Sun.
"This came as a shock to us, as no one expected to detect these object at radio wavelengths and with the present generation of radio telescopes," said Filipovic.
"We have been holding up our findings for some 3 years until we were 100 percent sure that they are indeed Planetary Nebulae," he added.