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Carbon to Helium Ratio in the Wind of Central Stars of Planetary Nebulae with WC Spectrum

Published online by Cambridge University Press:  07 August 2017

J.A. De Freitas Pacheco
Affiliation:
Instituto Astron⊚mico e Geofísico, Universidade de São Paulo, Brazil
R.D.D. Costa
Affiliation:
Instituto Astron⊚mico e Geofísico, Universidade de São Paulo, Brazil
F.X. De Araújo
Affiliation:
Observatório Nacional - CNPq, Rio de Janeiro, Brazil
D. Petrini
Affiliation:
Observatoire de la C⊚te D'Azur, Nice, France

Abstract

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We present C/He ratios in the wind of a sample of 5 central stars of planetary nebulae having WC spectrum. The resulting values are comparable to those observed in population I WR stars.

Type
Near Stellar Environments
Copyright
Copyright © Kluwer 1992 

References

REFERENCES

Castor, J., Lutz, J.H., Seaton, M.J. 1981, Mon. Not. R. astr. Soc. 194, 547 CrossRefGoogle Scholar
Cerruti-Sola, M., Pcrinotto, M. 1985, Ap.J. 291, 237 Google Scholar
Clegg, R.E.S. 1989 in Planetary Nebulae ed. Torres-Peimbert, S. - Reidel, Dordrecht, pg. 139 Google Scholar
De Freitas Pacheco, J.A., Araujo, F.X., Costa, R.D.D., Petrini, D. 1991 - in preparation Google Scholar
De Freitas Pacheco, J.A., Machado, M.A.D. 1988, Astron. J. 96, 365 Google Scholar
Kaler, J.B., Shaw, R.A., Feibelmann, W.A., Lutz, J.H. 1989, Ap.J. Supp. 70, 213 Google Scholar
Torres, A.V. 1988, Ap.J. 325, 759 Google Scholar