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Chemical abundances of cold stars in binary nuclei of Abell 35–type Planetary Nebulae

Published online by Cambridge University Press:  25 May 2016

G. Jasniewicz ,
F. Thévenin  and
A. Acker
G. Jasniewicz
Affiliation:
1Observatoire de Strasbourg 2GRAAL Montpellier
F. Thévenin
Affiliation:
3Observatoire de Nice
A. Acker
Affiliation:
1Observatoire de Strasbourg

Extract

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Jasniewicz et al. (1994) have announced and started in 1994 a program of chemical analysis of the G-stars at the centre of Abell 35-type planetary nebulae. First results concerning BD-22° 3467 and HD 112313 located respectively at the centre of Abell 35 and LoTr5 have been published by Jasniewicz et al. (1996) and Thévenin & Jasniewicz (1996).

Type
III. Central Stars
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 111
Copyright
Copyright © Kluwer 1997 

References

Bond, H.E., 1993, In: Barstow, M.A. (ed) White Dwarfs: Advances in Observation and Theory. Kluwer, Dordrecht, p. 85.Google Scholar
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