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Angular Momentum Loss in Post-Main Sequence Stellar Evolution Through the PN Stage
Published online by Cambridge University Press: 07 August 2017
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A simple analytical model can explain the large angular momentum loss which a star suffers in its post-main-sequence evolution up to the white dwarf stage.
- Type
- IV. Planetary Nebulae Connection: Evolution from the AGB
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- Copyright
- Copyright © Kluwer 1993
References
Greenstein, J.L., Boksenberg, A., Carswell, R., and Shortridge, K. (1977), ApJ
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