Inlists for paper: Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae

MESA (v10108) inlists for the models shown the "Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae" Letter (1903.02135). The inlists reproduce both the single and merger model. Contents: FiducialMergersPPISN.tar.gz doubleMass evolveMerged evolveSingle preMSmodel README We also attach the single and merger MESA models at the moment where the central temperature is close to 10^9 K. These models where used to estimate the properties of the star, particularly core and envelope masses, as well as element abundances. mergerAtLogTc9.data singleAtLogTc9.data

Country

Netherlands

Related Organizations

University of Birmingham
United Kingdom
University of Amsterdam
Netherlands
Monash University
Australia
University of Oxford
United Kingdom
University of Chinese Academy of Sciences
China (People's Republic of)

Impact byBIP!

	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