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Carbon- and Oxygen-Rich Progenitors of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

H.J. Habing  and
J.A.D.L. Blommaert
H.J. Habing
Affiliation:
Sterrewacht Leiden, P.O. Box 9513, 2300 RA Leiden, The Netherlands
J.A.D.L. Blommaert
Affiliation:
Sterrewacht Leiden, P.O. Box 9513, 2300 RA Leiden, The Netherlands

Extract

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This review concerns stars on the Asymptotic Giant Branch that are about to develop into planetary nebulae (=PNe). They are still termed “stars”, and properly so, and yet they have already, in statu nascendi, the structure of a PN. There are two different kinds: oxygen-rich stars (spectral class: M) and carbon-rich stars (spectral class: C).

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 243 - 250
Copyright
Copyright © Kluwer 1993 

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