Abstract
(Abridged) We determine the yields of Na to Ni for Type II supernovae (SNe II) and the yield patterns of the same elements for Type Ia supernovae (SNe Ia) and very massive (>100 M_sun) stars (VMS) using a phenomenological model of stellar nucleosynthesis and the data on a number of stars with -4
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CITATION STYLE
APA
Qian, Y. ‐Z., & Wasserburg, G. J. (2002). Determination of Nucleosynthetic Yields of Supernovae and Very Massive Stars from Abundances in Metal‐Poor Stars. The Astrophysical Journal, 567(1), 515–531. https://doi.org/10.1086/338277
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