Inlists and initial models for simulating post-merger evolution of double ONe WD merger remnant (arXiv: 2308.10695 ). Folder includes initial models of merger remnants and and inlists for calculating their post merger evolution, and the corresponding nuclear reaction network. Folder named "src" includes "run_star_extras.f90", in which different wind mass-loss prescriptions and stopping conditions can be setted, and also opacity tables
Recent observations suggest that some Type Ia supernovae (SNe Ia) originate from the merging of two ...
Abstract. Recent studies have shown that for suitable initial conditions both super- and sub-Chandra...
Context. The coalescence of two white dwarfs is the final outcome of a sizeable fraction of binary s...
Inlists and initial models for simulating post-merger evolution of ONe WD + CO WD pairs. Folder in...
Inlists and initial models for simulating post-merger evolution of CO WD + He WD pairs. Description...
Inlists and data for "Evolution models of helium white dwarf-main-sequence star merger remnants: the...
We systematically explore the evolution of the merger of two carbon-oxygen (CO) white dwarfs. The dy...
In double white dwarf (WD) systems with sufficiently short initial orbital periods, angular momentum...
We present a large parameter study where we investigate the structure of white dwarf (WD) merger rem...
The merger of two carbon-oxygen white dwarfs can lead either to a spectacular transient, stable nucl...
The final outcome of white dwarf mergers across the entire merger parameter space is still relativel...
We carry out a comprehensive smooth particle hydrodynamics simulation survey of double-degenerate wh...
The merger of two white dwarfs (WDs) creates a differentially rotating remnant which is unstable to ...
The merger of two carbon-oxygen white dwarfs (CO WDs) can either create a more massive WD, lead to c...
In this thesis, I describe the evolution following the merger of two helium white dwarfs. Three sets...
Recent observations suggest that some Type Ia supernovae (SNe Ia) originate from the merging of two ...
Abstract. Recent studies have shown that for suitable initial conditions both super- and sub-Chandra...
Context. The coalescence of two white dwarfs is the final outcome of a sizeable fraction of binary s...
Inlists and initial models for simulating post-merger evolution of ONe WD + CO WD pairs. Folder in...
Inlists and initial models for simulating post-merger evolution of CO WD + He WD pairs. Description...
Inlists and data for "Evolution models of helium white dwarf-main-sequence star merger remnants: the...
We systematically explore the evolution of the merger of two carbon-oxygen (CO) white dwarfs. The dy...
In double white dwarf (WD) systems with sufficiently short initial orbital periods, angular momentum...
We present a large parameter study where we investigate the structure of white dwarf (WD) merger rem...
The merger of two carbon-oxygen white dwarfs can lead either to a spectacular transient, stable nucl...
The final outcome of white dwarf mergers across the entire merger parameter space is still relativel...
We carry out a comprehensive smooth particle hydrodynamics simulation survey of double-degenerate wh...
The merger of two white dwarfs (WDs) creates a differentially rotating remnant which is unstable to ...
The merger of two carbon-oxygen white dwarfs (CO WDs) can either create a more massive WD, lead to c...
In this thesis, I describe the evolution following the merger of two helium white dwarfs. Three sets...
Recent observations suggest that some Type Ia supernovae (SNe Ia) originate from the merging of two ...
Abstract. Recent studies have shown that for suitable initial conditions both super- and sub-Chandra...
Context. The coalescence of two white dwarfs is the final outcome of a sizeable fraction of binary s...
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