Fate of merging double white dwarfs. II - Numerical method

Details Fate of merging double white dwarfs. II - Numerical method Fate of merging double white dwarfs. II - Numerical method

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...311..214h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 311, Dec. 1, 1986, p. 214-225.

Statistics

Computation

14

Computational Astrophysics, Double Stars, Stellar Evolution, Supernovae, White Dwarf Stars, Accretion Disks, Density Distribution, Kepler Laws, Stellar Models, Stellar Rotation, Three Dimensional Models, Two Dimensional Models

Scientific paper

The authors present a new numerical method for constructing models of double white dwarf binary systems and central white dwarf-heavy disk systems. These two types of models were constructed in paper I to examine whether or not the merging white dwarfs result in a Type I supernova. In the present paper, the authors present details of their method for computing three-dimensional models of double white dwarfs with zero-temperature equation of state, and also a computational method for two-dimensional models of a system consisting of a central white dwarf and a surrounding heavy disk.

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