Red novae, stellar mergers in binary and triple systems, and bipolar nebulae
arxiv(2024)
摘要
Red novae are transients powered by collisions of non-compact stars. Among
their progenitors are systems of evolved subgiants and giants stars. Remnants
of such red novae display bipolar structures which have remarkably close
characteristics to many post-AGB or pre-PN systems. It is important to ask (and
eventually verify) whether some of the less-known post-main-sequence objects
(mis-)classified as pre-PNe can be merger remnants similar to the red nova
remnants.
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