VizieR Online Data Catalog: Massive runaway and walkaway stars models (Renzo+, 2019)

Each file contains the output of our population synthesis simulations (see Table 1). The data files include both systems remaining bound and those that are disrupted. Each system is logged at the time of the first SN and we store initial values of masses and period, the pre-cor-collapse and post-core collapse masses, period, eccentricity, separation, and information on the explosion (kick amplitude and direction, fallback fraction) and the pre-CC and post-CC orbital and kinematic properties. We also provide the time each system spends in phases with at least one of the two stars on the main sequence.

(2 data files).