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Abundances for a large sample of galactic Planetary Nebulae

Published online by Cambridge University Press:  25 May 2016

V. V. Golovaty  and
Yu.F. Malkov
V. V. Golovaty
Affiliation:
1Astronomical Observatory of Lviv State University, Lviv, Ukraine
Yu.F. Malkov
Affiliation:
2Crimean Astrophysical Observatory, Nauchny, Crimea, Ukraine

Extract

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We present a database on the chemical composition of 200 planetary nebulae (PNe) in our Galaxy. Abundances of He, C, N, O, Ne, Mg, Si, S, and Ar are found for 175, 64, 190, 200, 170, 13, 40, 173, and 187 PNe respectively. The abundances for all PNe are obtained with the same atomic data and by the same method of abundance determination, so the database is highly homogeneous. The method of the determination of nebular abundances based on a photoionization model grid is described by Golovaty et al. (1993). Observational data have been compiled from 105 papers published in 1976–1994. For most of PNe in our sample, the distances and central star masses are determined as well (Malkov, this volume).

Type
VII. Planetary Nebulae in the Galactic Context
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 408
Copyright
Copyright © Kluwer 1997 

References

Chiappini, C., and Maciel, W.J., 1994, Astron. Astrophys., 288, 921.Google Scholar
Golovaty, V.V., Dmiterko, V.I., Malkov, Yu.F., and Rokach, O.V., 1993, Astron. Zhurn., 70, 691.Google Scholar
Groenewegen, M.A.T., and de Jong, T., 1994, Astron. Astrophys., 282, 127.Google Scholar
Groenewegen, M.A.T., van den Hoek, L.B., and de Jong, T., 1995, Astron. Astrophys., 293, 381.Google Scholar