An international team of researchers, including scientists from the Instituto de Astrofísica de Canarias, has published a detailed study of the evolution of the nebula surrounding the symbiotic star R Aquarii. The study involved observations from telescopes at the Roque de los Muchachos Observatory, La Palma, and Chile taken over the course of more than two decades.
In astronomical terms, at 600 light years away, the nebula around R Aquarii is relatively close. The symbiotic star is made up of a red giant and a white dwarf that have interacted over centuries to form the magnificent surrounding nebula from material ejected from the system.
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In astronomical terms, at 600 light years away, the nebula around R Aquarii is relatively close. The symbiotic star is made up of a red giant and a white dwarf that have interacted over centuries to form the magnificent surrounding nebula from material ejected from the system.
Continued...
Source