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Red novae, stellar mergers in binary and triple systems, and bipolar nebulae
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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.
Forward citations
Cited by 2 Pith papers
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Mass-feeding of jet-launching white dwarfs in grazing and common envelope evolution
White dwarfs entering a giant's envelope may grow a one-solar-radius accretion disk that launches jets powered by gravitational energy, explaining jet-shaped planetary nebulae and luminous red novae.
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Constraining the physical structure of the circumstellar environment of V838 Monocerotis remnant
A torus, jets, and inner ellipsoid model reproduces most H-band interferometry and low polarization of V838 Mon, but leaves the K-band closure phases unexplained.
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