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Title: The Role of Dredge-up in Double White Dwarf Mergers

Abstract

We present the results of an investigation of the dredge-up and mixing during the merger of two white dwarfs (WDs) with different chemical compositions by conducting hydrodynamic simulations of binary mergers for three representative mass ratios. In all the simulations, the total mass of the two WDs is $$\lesssim$$1.0 M. Mergers involving a CO and a He WD have been suggested as a possible formation channel for R Coronae Borealis (RCB)–type stars, and we are interested in testing if such mergers lead to conditions and outcomes in agreement with observations. Even if the conditions during the merger and subsequent nucleosynthesis favor the production of 18O, the merger must avoid dredging up large amounts of 16O, or else it will be difficult to produce sufficient 18O to explain the oxygen ratio observed to be of order unity. Here, we performed a total of nine simulations using two different grid-based hydrodynamics codes using fixed and adaptive meshes and one smooth particle hydrodynamics (SPH) code. We find that in most of the simulations, >10-2 M of 16O is indeed dredged up during the merger. However, in SPH simulations where the accretor is a hybrid He/CO WD with a ~0.1 M layer of helium on top, we find that no 16O is being dredged up, while in the q = 0.8 simulation <10-4 M of 16O has been brought up, making a WD binary consisting of a hybrid CO/He WD and a companion He WD an excellent candidate for the progenitor of RCB stars.

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [4]; ORCiD logo [5]; ORCiD logo [5];  [6]; ORCiD logo [3];  [3]
  1. Univ. of the Virgin Islands, St. Thomas, VI (United States). College of Science and Math
  2. Los Alamos National Lab. (LANL), Los Alamos, NM (United States); Southern Utah Univ., Cedar City, UT (United States)
  3. Louisiana State Univ., Baton Rouge, LA (United States). Dept. of Physics and Astronomy
  4. Indiana Univ., Kokomo, IN (United States). School of Sciences
  5. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  6. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Publication Date:
Research Org.:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
USDOE National Nuclear Security Administration (NNSA); Australian Research Council (ARC); National Aeronautic and Space Administration (NASA); National Science Foundation (NSF)
OSTI Identifier:
1469529
Report Number(s):
LA-UR-17-25739
Journal ID: ISSN 1538-4357
Grant/Contract Number:  
AC52-06NA25396; NNX10AC72G; NNX15AP95A; AST-1240655; TG-AST090104; GAST110034
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 862; Journal Issue: 1; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; binaries: close; hydrodynamics; methods: numerical; white dwarfs

Citation Formats

Staff, Jan. E., Wiggins, Brandon Kerry, Marcello, Dominic, Motl, Patrick M., Even, Wesley Paul, Fryer, Chris Lee, Raskin, Cody, Clayton, Geoffrey C., and Frank, Juhan. The Role of Dredge-up in Double White Dwarf Mergers. United States: N. p., 2018. Web. doi:10.3847/1538-4357/aaca3d.
Staff, Jan. E., Wiggins, Brandon Kerry, Marcello, Dominic, Motl, Patrick M., Even, Wesley Paul, Fryer, Chris Lee, Raskin, Cody, Clayton, Geoffrey C., & Frank, Juhan. The Role of Dredge-up in Double White Dwarf Mergers. United States. doi:https://doi.org/10.3847/1538-4357/aaca3d
Staff, Jan. E., Wiggins, Brandon Kerry, Marcello, Dominic, Motl, Patrick M., Even, Wesley Paul, Fryer, Chris Lee, Raskin, Cody, Clayton, Geoffrey C., and Frank, Juhan. Fri . "The Role of Dredge-up in Double White Dwarf Mergers". United States. doi:https://doi.org/10.3847/1538-4357/aaca3d. https://www.osti.gov/servlets/purl/1469529.
@article{osti_1469529,
title = {The Role of Dredge-up in Double White Dwarf Mergers},
author = {Staff, Jan. E. and Wiggins, Brandon Kerry and Marcello, Dominic and Motl, Patrick M. and Even, Wesley Paul and Fryer, Chris Lee and Raskin, Cody and Clayton, Geoffrey C. and Frank, Juhan},
abstractNote = {We present the results of an investigation of the dredge-up and mixing during the merger of two white dwarfs (WDs) with different chemical compositions by conducting hydrodynamic simulations of binary mergers for three representative mass ratios. In all the simulations, the total mass of the two WDs is $\lesssim$1.0 M⊙. Mergers involving a CO and a He WD have been suggested as a possible formation channel for R Coronae Borealis (RCB)–type stars, and we are interested in testing if such mergers lead to conditions and outcomes in agreement with observations. Even if the conditions during the merger and subsequent nucleosynthesis favor the production of 18O, the merger must avoid dredging up large amounts of 16O, or else it will be difficult to produce sufficient 18O to explain the oxygen ratio observed to be of order unity. Here, we performed a total of nine simulations using two different grid-based hydrodynamics codes using fixed and adaptive meshes and one smooth particle hydrodynamics (SPH) code. We find that in most of the simulations, >10-2 M⊙ of 16O is indeed dredged up during the merger. However, in SPH simulations where the accretor is a hybrid He/CO WD with a ~0.1 M⊙ layer of helium on top, we find that no 16O is being dredged up, while in the q = 0.8 simulation <10-4 M⊙ of 16O has been brought up, making a WD binary consisting of a hybrid CO/He WD and a companion He WD an excellent candidate for the progenitor of RCB stars.},
doi = {10.3847/1538-4357/aaca3d},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 862,
place = {United States},
year = {2018},
month = {7}
}

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    Works referencing / citing this record:

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