behind AD 1181 due to its close proximity, but its was ruled out because of its age and close observations. The team said that this left"no other viable candidate known for the remnant."
Pa 30 had previously been considered to be created as the result of a collision between two dense stars called white dwarfs. These degenerate stars form when smallerburn up their nuclear fuel and begin to dim towards the end of their lives. This results in the loss of their outer layers and a remaining core of dense material.
If that is indeed the cause of this nebula and SN 1181, it marks only the second time such a collision has been discovered in our galaxy.
It was spotted 840 years ago but actually occurred how long ago?
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