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Long-term Evolution and Appearance of Type Iax Postgenitor Stars

Zhang, Michael and Fuller, Jim and Schwab, Josiah and Foley, Ryan J. (2019) Long-term Evolution and Appearance of Type Iax Postgenitor Stars. Astrophysical Journal, 872 (1). Art. No. 29. ISSN 1538-4357. http://resolver.caltech.edu/CaltechAUTHORS:20190207-102750197

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Abstract

Type Iax supernovae may arise from failed explosions of white dwarfs (WDs) that leave behind a bound remnant (i.e., a "postgenitor" star) that could be identified in wide field surveys. To understand their observational signatures, we simulate these WD postgenitors from shortly after explosion until they move back down the WD cooling track, and we consider several possible WD masses and explosion energies. To predict the peculiar surface abundances of the WD postgenitors, our models take into account gravitational settling and radiative levitation. We find that radiative levitation is significant at temperatures above a mass-dependent critical temperature, typically in the range T_(eff) ≈ (50–100) × 10^3 K, significantly increasing surface abundances of iron group elements. Due to enhanced iron group opacity compared to normal WDs, the postgenitor peak luminosity and cooling timescale depend sensitively on mass, with more massive WDs becoming brighter but cooling much faster. We discuss our results in light of recently discovered hypervelocity WDs with peculiar surface compositions, finding that our low-mass postgenitor models match many of their observational characteristics. Finally, we explore the effects of thermohaline diffusion, tentatively finding that it strongly suppresses abundance enhancements created by radiative levitation, but more realistic modeling is required to reach a firm conclusion.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4357/aafb34DOIArticle
https://arxiv.org/abs/1812.08793arXivDiscussion Paper
ORCID:
AuthorORCID
Zhang, Michael0000-0002-0659-1783
Fuller, Jim0000-0002-4544-0750
Schwab, Josiah0000-0002-4870-8855
Additional Information:© 2019 The American Astronomical Society. Received 2018 October 31; revised 2018 December 27; accepted 2018 December 28; published 2019 February 7. We thank Ken Shen, Evan Bauer, and Lars Bildsten for useful discussions, and we thank the referee for a very constructive and thorough report. This work was supported by the Heising-Simons Foundation through grant #2017-274. Support for this work was provided by NASA through Hubble Fellowship grant #HST-HF2-51382.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. This research made use of NASA's Astrophysics Data System. R.J.F. is supported in part by NSF grant AST-1518052, the Gordon & Betty Moore Foundation, and by a fellowship from the David and Lucile Packard Foundation. Software: MESA, py_mesa_reader, numpy, scipy, matplotlib.
Funders:
Funding AgencyGrant Number
Heising-Simons Foundation2017-274
NASA Hubble FellowshipHST-HF2-51382.001-A
NASANAS5-26555
NSFAST-1518052
Gordon and Betty Moore FoundationUNSPECIFIED
David and Lucile Packard FoundationUNSPECIFIED
Subject Keywords:ISM: supernova remnants – stars: evolution – supernovae: general – white dwarfs
Record Number:CaltechAUTHORS:20190207-102750197
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190207-102750197
Official Citation:Michael Zhang et al 2019 ApJ 872 29
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:92754
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:07 Feb 2019 18:38
Last Modified:07 Feb 2019 18:38

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