
MESA inlists and other input files used for the paper "Evolution of Binaries Containing a Hot Subdwarf and a White Dwarf to Double White Dwarfs and Double Detonation Supernovae with Hypervelocity Runaway Stars." These files were generated using a modified MESA version r23.05.1. A modification was made to the binary_mdot.f90 file to alter the composition of the accretion stream, converting the mass fraction of H to He throughout accretion. This adjustment was implemented to reduce computational time associated with modeling H novae, as the study focuses on He novae and supernovae. For further details, please refer to Section 2 of the paper. The modified binary_mdot.f90 file is also included in this repository.
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
