Energy and Angular Momentum Deposition During Common Envelope Evolution

Abstract

I consider three processes which enhance mass loss rate from a common envelope of a giant star with a main sequence or a white dwarf companion spiraling-in inside its envelope. I consider deposition of orbital energy and orbital angular momentum to the giant's envelope, and in more detail the formation of jets by an accreting companion and their propagation in the envelope. I find that in many cases the deposition of orbital angular momentum to the envelope may be more important to the mass loss process than the deposition of orbital energy. Jets blown by an accreting companion, in particular a white dwarf, orbiting inside the outer regions of the giant's envelope may also dominate over orbital energy deposition at early stage of the common envelope evolution. These imply that studies which ignore the deposition of angular momentum to the envelope and the effects of the accreting companion may reach wrong conclusions.

arXiv commentWork prepared to IAU Colloquium 194: Compact Binaries in the Galaxy and Beyond, La Paz, Baja California Sur, Mexico, November 17, 2003

References in corpus (14)

• The Origin of Subdwarf B Star (I): the Formation Channels
• The origin of sdB stars (II)
• A Wide Symbiotic Channel to Type Ia Supernovae
• The Formation of Very Narrow Waist Bipolar Planetary Nebulae
• Hubble Space Telescope Spectroscopy of V471 Tauri: Oversized K Star, Paradoxical White Dwarf
• On the Formation of Helium Double Degenerate Stars and Pre-Cataclysmic Variables
• Black hole formation via hypercritical accretion during common envelope evolution
• Collimated Fast Winds in Wide Binary Progenitors of Planetary Nebulae
• Hydrodynamical Simulations of the Stream-Core Interaction in the Slow Merger of Massive Stars
• PG1115+166 - a long period DA+DB binary
• Stellar Structure and Mass Loss on the Upper AGB
• X-Ray Emission from Central Binary Systems of Planetary Nebulae
• Envelope Ejection: an Alternative Process for some Early Case B Binaries
• Comments on the Final Orbital Separation in Common Envelope Evolution

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• Common Envelope Evolution: Where we stand and how we can move forward
• A Circumbinary Disk in the Final Stages of Common Envelope and the Core-Degenerate Scenario for Type Ia Supernovae
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• Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226
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• Close stellar binary systems by grazing envelope evolution
• Companion-launched jets and their effect on the dynamics of common envelope interaction simulations
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• Formation channels of single and binary stellar-mass black holes
• The demographics of neutron star - white dwarf mergers: rates, delay-time distributions and progenitors
• Explaining iPTF14hls as a common envelope jets supernova
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• Accretion Disk Assembly During Common Envelope Evolution: Implications for Feedback and LIGO Binary Black Hole Formation
• The common envelope jets supernova (CEJSN) r-process scenario
• Using Kinematic Properties of Pre-Planetary Nebulae to Constrain Engine Paradigms
• A carbon dwarf wearing a Necklace: first proof of accretion in a post-common-envelope binary central star of a planetary nebula with jets
• Planet formation from the ejecta of common envelopes
• Energy transport by convection in the common envelope evolution
• A two-stage formalism for common-envelope phases of massive stars
• Understanding Compact Object Formation and Natal Kicks. IV. The case of IC 10 X-1
• Dynamics of jets during the Common Envelope phase
• Simulating a binary system that experiences the grazing envelope evolution
• Disk formation and jet inclination effects in Common Envelopes
• Common envelope jets supernova (CEJSN) impostors resulting from a neutron star companion
• Simulating the Onset of Grazing Envelope Evolution of Binary Stars
• Radiating the hydrogen recombination energy during common envelope evolution
• Possible Implications of the Planet Orbiting the Red Horizontal Branch Star HIP 13044
• Operation of the jet feedback mechanism (JFM) in intermediate luminosity optical transients (ILOTs)
• Energizing the last phase of common envelope removal
• Merger by Migration at the Final Phase of Common Envelope Evolution
• Jets in Common Envelopes: a low mass main sequence star in a red giant
• Common Envelope Evolution on the Asymptotic Giant Branch: Unbinding within a Decade?
• Launching jets from accretion belts
• On the Common Envelope Efficiency
• Accreting White Dwarfs among the Planetary Nebulae Most Luminous in [O III]5007 Emission
• SCATTER: A New Common Envelope Formalism
• Spinning-Up the Envelope Before Entering a Common Envelope Phase
• Grazing envelope evolution toward Type IIb supernovae
• Common Envelope Evolution of Massive Stars
• High-speed knots in the hourglass shaped planetary nebula Hubble 12
• A Triple Star Origin For T Pyx and Other Short-Period Recurrent Novae
• Jets from main sequence and white dwarf companions during common envelope evolution
• Panchromatic HST/WFC3 Imaging Studies of Young, Rapidly Evolving Planetary Nebulae. I. NGC 6302
• The Class of Jsolated Stars and Luminous Planetary Nebulae in old stellar populations
• A survey for post common-envelope binary stars using GALEX and SDSS photometry
• Hypercritical accretion during common envelopes in triples leading to binary black holes in the pair-instability-supernova mass gap
• The Morphology of the Outflow in the Grazing Envelope Evolution
• Binary Systems of core collapse supernova polluting a giant companion
• A companion star launching jets in the wind acceleration zone of a giant star
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• On the nature of jets from a main sequence companion at the onset of common envelope evolution
• Jsolated Stars of Low Metallicity