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Pre-supernova outbursts via wave heating in massive stars – II. Hydrogen-poor stars

Fuller, Jim and Ro, Stephen (2018) Pre-supernova outbursts via wave heating in massive stars – II. Hydrogen-poor stars. Monthly Notices of the Royal Astronomical Society, 476 (2). pp. 1853-1868. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20180510-083538543

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Abstract

Pre-supernova (SN) outbursts from massive stars may be driven by hydrodynamical wave energy emerging from the core of the progenitor star during late nuclear-burning phases. Here, we examine the effects of wave heating in stars containing little or no hydrogen, i.e. progenitors of Type IIb/Ib SNe. Because there is no massive hydrogen envelope, wave energy is thermalized near the stellar surface where the overlying atmospheric mass is small but the optical depth is large. Wave energy can thus unbind this material, driving an optically thick, super-Eddington wind. Using 1D hydrodynamic MESAsimulations of ∼5 M⊙ He stars, we find that wave heating can drive pre-SN outbursts composed of a dense wind whose mass-loss rate can exceed ∼0.1 M⊙ yr^(−1). The wind terminal velocities are a few 100 km s^(−1), and outburst luminosities can reach ∼10^6 L⊙. Wave-driven outbursts may be linked with observed or inferred pre-SN outbursts of Type Ibn/transitional/transformational SNe, and pre-SN wave-driven mass loss is a good candidate to produce these types of SNe. However, we also show that non-linear wave breaking in the core of the star may prevent such outbursts in stars with thick convective helium-burning shells. Hence, only a limited subset of SN progenitors is likely to experience wave-driven pre-SN outbursts.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/sty369DOIArticle
https://arxiv.org/abs/1710.04251arXivDiscussion Paper
ORCID:
AuthorORCID
Fuller, Jim0000-0002-4544-0750
Additional Information:© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2018 February 8. Received 2018 February 8; in original form 2017 October 1. Published: 14 February 2018. JF acknowledges partial support from NSF under grant no. AST-1205732 and through a Lee DuBridge Fellowship at Caltech. This research was supported in part by the National Science Foundation under grant no. NSF PHY-1125915, and by the Gordon and Betty Moore Foundation through grant GBMF5076.
Group:TAPIR, Walter Burke Institute for Theoretical Physics
Funders:
Funding AgencyGrant Number
NSFAST-1205732
Lee DuBridge FellowshipUNSPECIFIED
NSFPHY-1125915
Gordon and Betty Moore FoundationGBMF5076
Subject Keywords:circumstellar matter – stars: massive – stars: mass-loss – stars: oscillations – supernovae: general – stars: winds, outflows
Record Number:CaltechAUTHORS:20180510-083538543
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20180510-083538543
Official Citation:Jim Fuller, Stephen Ro; Pre-supernova outbursts via wave heating in massive stars – II. Hydrogen-poor stars, Monthly Notices of the Royal Astronomical Society, Volume 476, Issue 2, 11 May 2018, Pages 1853–1868, https://doi.org/10.1093/mnras/sty369
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:86326
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:10 May 2018 16:58
Last Modified:10 May 2018 16:58

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