{ "id": "1204.3173", "version": "v2", "published": "2012-04-14T13:45:45.000Z", "updated": "2012-05-05T13:25:07.000Z", "title": "Merger by Migration at the Final Phase of Common Envelope Evolution", "authors": [ "Noam Soker" ], "comment": "New Astronomy, in press", "categories": [ "astro-ph.SR" ], "abstract": "I find the common envelope (CE) energy formalism, the CE \\alpha-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 \\alpha-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 \\alpha-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.", "revisions": [ { "version": "v2", "updated": "2012-05-05T13:25:07.000Z" } ], "analyses": { "keywords": [ "common envelope evolution", "final phase", "final orbital separation", "angular momentum", "ce evolution" ], "tags": [ "journal article" ], "publication": { "doi": "10.1016/j.newast.2012.05.001", "journal": "New Astronomy", "year": 2013, "month": "Jan", "volume": 18, "pages": 18 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1110927, "adsabs": "2013NewA...18...18S" } } }