Long-Sought Remnants of Massive Stars Found

Long-Sought Remnants of Massive Stars Found
An optical image from the 0.6-m University of Michigan/CTIO Curtis Schmidt telescope of the brightest Radio Planetary Nebula in the Small Magellanic Cloud, JD 04. The inset box shows a portion of this image overlaid with radio contours from the Australia Telescope Compact Array. The planetary nebula is a glowing record of the final death throes of the star. (Image credit: Magellanic Cloud Emission Line Survey (MCELS)/E. Crawford & S. Griffith.)

A new class of cosmic object ? dubbed a ?super planetarynebula? ? has been identified by astronomers.

Planetary nebulas are shellsof gas and dust expelled by stars near the end of their lives and aretypically seen around stars comparable or smaller in size than the sun. Thesenebulas aren't related to planets ? the name arose because they resembled giantplanets when viewed through early telescopes.

"This came as a shock to us," said MiroslavFilipovic of the University of Western Sydney in Australia, "as no oneexpected to detect these object at radio wavelengths and with the present generationof radio telescopes."

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