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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

M. Villata
M. Villata*
Affiliation:
Istituto di Fisica Generale, Università di Torino, Via Pietro Giuria 1, I-10125 Torino, Italy

Extract

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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
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 368
Copyright
Copyright © Kluwer 1993 

References

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