Using a powerful telescope, scientists view spiral pattern of gaseous emissions around LL Pegasi and its companion star. An international team of astronomers has observed a striking spiral pattern in the gas surrounding a red giant star named LL Pegasi and its companion star 3,400 light-years from Earth using ALMA. “What we are seeing in splendid detail with these observations is the final act of a dying red giant star, as it sheds most of its gaseous bulk in a strong, outflowing wind,” said Mark Morris, UCLA professor of physics and astronomy.
After comparing their telescopic observations with computer simulations, the astronomers concluded that a highly elliptical orbit is responsible for the shape of the gaseous emi...
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