Appendix/Ramblings/BdHN: Difference between revisions

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=Binary-driven Hpernovae=
=Binary-driven Hypernovae=
The material presented here builds on our separate discussion of [[Appendix/Ramblings/TurningPoints#Close_Binary_Stars|close binary stars]].
The material presented here builds on our separate discussion of [[Appendix/Ramblings/TurningPoints#Close_Binary_Stars|close binary stars]].


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==Setup==
==Setup==


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=Critique=
=Critique=
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C. See, for example, the expression for L_1 immediately following Eq. (1) on p. 165 of Darwin, G. H. (1906, Philosophical Transactions of the Royal Society A, Vol. 206, 161).
C. See, for example, the expression for L_1 immediately following Eq. (1) on p. 165 of Darwin, G. H. (1906, Philosophical Transactions of the Royal Society A, Vol. 206, 161).
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==Other==
==Other==
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<li>Ill-advised to refer to the ''new'' NS as "&nu;NS" because, in this context, readers might reasonably associate the greek letter, &nu;, with neutrinos. </li>
<li>Ill-advised to refer to the ''new'' NS as "&nu;NS" because, in this context, readers might reasonably associate the greek letter, &nu;, with neutrinos. </li>
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=See Also=
=See Also=

Latest revision as of 12:59, 4 July 2023


Binary-driven Hypernovae

The material presented here builds on our separate discussion of close binary stars.

HIDDEN as of 4 July 2023.





See Also

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