Inlists and initial models for simulating post-merger evolution of ONe WD + CO WD pairs. Folder includes initial models of merger remnants and and inlists for calculating their post merger evolution, and the corresponding nuclear reaction network and opacity tables. Folder named "fiducial_models" includes initial models (after energy injection) of ONe+CO WD and ONe+HeCO WD merger remnants (including by considering different initial entropy profiles and nuclear reaction networks). Folder named "rotating _models" includes ONe+CO WD merger remnants with differential rotational velocities. Folder named "src" includes "run_star_extras.f90", in which different wind mass-loss prescriptions and stopping conditions can be setted
The R Coronae Borealis (RCB) stars are hydrogen-deficient, variable stars that are most likely the r...
Context. The coalescence of two white dwarfs is the final outcome of a sizeable fraction of binary s...
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 double ONe WD merger remnant (arX...
Inlists and initial models for simulating post-merger evolution of CO WD + He WD pairs. Description...
We systematically explore the evolution of the merger of two carbon-oxygen (CO) white dwarfs. The dy...
We present a large parameter study where we investigate the structure of white dwarf (WD) merger rem...
We carry out a comprehensive smooth particle hydrodynamics simulation survey of double-degenerate wh...
In double white dwarf (WD) systems with sufficiently short initial orbital periods, angular momentum...
The merger of two carbon-oxygen white dwarfs can lead either to a spectacular transient, stable nucl...
Inlists and data for "Evolution models of helium white dwarf-main-sequence star merger remnants: the...
The merger of two white dwarfs (WDs) creates a differentially rotating remnant which is unstable to ...
The final outcome of white dwarf mergers across the entire merger parameter space is still relativel...
In this thesis, I describe the evolution following the merger of two helium white dwarfs. Three sets...
The merger of two carbon-oxygen white dwarfs (CO WDs) can either create a more massive WD, lead to c...
The R Coronae Borealis (RCB) stars are hydrogen-deficient, variable stars that are most likely the r...
Context. The coalescence of two white dwarfs is the final outcome of a sizeable fraction of binary s...
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 double ONe WD merger remnant (arX...
Inlists and initial models for simulating post-merger evolution of CO WD + He WD pairs. Description...
We systematically explore the evolution of the merger of two carbon-oxygen (CO) white dwarfs. The dy...
We present a large parameter study where we investigate the structure of white dwarf (WD) merger rem...
We carry out a comprehensive smooth particle hydrodynamics simulation survey of double-degenerate wh...
In double white dwarf (WD) systems with sufficiently short initial orbital periods, angular momentum...
The merger of two carbon-oxygen white dwarfs can lead either to a spectacular transient, stable nucl...
Inlists and data for "Evolution models of helium white dwarf-main-sequence star merger remnants: the...
The merger of two white dwarfs (WDs) creates a differentially rotating remnant which is unstable to ...
The final outcome of white dwarf mergers across the entire merger parameter space is still relativel...
In this thesis, I describe the evolution following the merger of two helium white dwarfs. Three sets...
The merger of two carbon-oxygen white dwarfs (CO WDs) can either create a more massive WD, lead to c...
The R Coronae Borealis (RCB) stars are hydrogen-deficient, variable stars that are most likely the r...
Context. The coalescence of two white dwarfs is the final outcome of a sizeable fraction of binary s...
Context. The coalescence of two white dwarfs is the final outcome of a sizeable fraction of binary s...