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Stellar Yields and Chemical Evolution

Published online by Cambridge University Press:  19 July 2016

Brad K. Gibson
Brad K. Gibson*
Affiliation:
Mount Stromlo & Siding Spring Observatories Weston Creek P.O., Weston, ACT, 2611 Australia

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Several speakers at this symposium have alluded to the zeroth-order agreement between the Type II supernovae (SNe) stellar yields, as predicted by the models of those most responsible for driving progress in the field - i.e. Arnett (1991,1996); Maeder (1992); Woosley & Weaver (1995); Langer & Henkel (1995); Thielemann et al. (1996), hereafter referred to as A91, A96, M92, WW95, LH95, and TNH96, respectively. It is important though for those entering (or indeed, already involved in!) the chemical evolution field to be cognizant of the fact that there are important first- and second-order differences between the yield compilations.

Type
Conference Papers in order of Presentation
Information
Symposium - International Astronomical Union , Volume 187: Cosmic Chemical Evolution , 2002 , pp. 159 - 163
Copyright
Copyright © 2002 

References

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