Properties of binary stellar models for an initial primary mass of 15 M⊙, conservative mass transfer and with variation of the initial secondary mass M2i and initial orbital period Porb.
|(M⊙)||(M⊙)||(M⊙)||(days)||(M⊙)||(103 K)||(103 K)|
Notes. The final mass of the primary and secondary, Mf1 and Mf2, and the amount of hydrogen in the envelope MH are given at the time of explosion, together with the luminosity log(L/L⊙) and effective temperature Teff of the primary and secondary at the onset of central carbon burning in the primary (except for model #4, where L2 and Teff, 2 refer to the last computed model of the secondary).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.