Merger by Migration at the Final Phase of Common Envelope Evolution

Abstract

I find the common envelope (CE) energy formalism, the CE α-prescription, to be inadequate to predict the final orbital separation of the CE evolution in massive envelopes. I find that when the orbital separation decreases to ~10 times the final orbital separation predicted by the CE α-prescription, the companion has not enough mass in its vicinity to carry away its angular momentum. The core-secondary binary system must get rid of its angular momentum by interacting with mass further out. The binary system interacts gravitationally with a rapidly-rotating flat envelope, in a situation that resembles planet-migration in protoplanetary disks. The envelope convection of the giant carries energy and angular momentum outward. The basic assumption of the CE α-prescription, that the binary system's gravitational energy goes to unbind the envelope, breaks down. Based on that, I claim that merger is a common outcome of the CE evolution of AGB and red super-giants stars with an envelope to secondary mass ratio of (M_env/M_2)>~5. I discuss some other puzzling observations that might be explained by the migration and merger processes.

New Astronomy, in press

References in corpus (4)

• Post-common-envelope binaries from SDSS. IX: Constraining the common-envelope efficiency
• Binary Star Origin of High Field Magnetic White Dwarfs
• Common Envelope Evolution Leading to Supernovae with Dense Interaction
• The filamentary Multi-Polar Planetary Nebula NGC 5189

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