Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-08T02:57:45.728Z Has data issue: false hasContentIssue false
  • English
  • Français

Simulations of a Population of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

G. Stasinska  and
R. Tylenda
G. Stasinska
Affiliation:
DAEC, Observatoire de Paris-Meudon, France
R. Tylenda
Affiliation:
DAEC, Observatoire de Paris-Meudon, France Copernicus Astronomical Center, Torun, Poland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present a simulation of the population of Galactic bulge planetary nebulae (GBPN), which matches the diagrams obtained from VLA radio observations. This simulation may not be the only one fitting the observed data, but it helps understanding the role of observational uncertainties and selection effects in the interpretation of observational diagrams.

Type
V. Planetary Nebulae Connection: Evolution to White Dwarfs
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 461 - 464
Copyright
Copyright © Kluwer 1993 

References

Blöcker, T., Schönberner, D. (1990) A&A 240, L11 Google Scholar
Schönberner, D. (1979) A&A 79, 108, (1983) APJ 272, 708 Google Scholar
Stasińska, G., Tylenda, R., Acker, A., Stenholm, B. (1989) A&A 247, 173 Google Scholar
Stasińska, G., Fresneau, A., Gameiro, G.F., Acker, A. (1991) A&A 252, 762 Google Scholar
Zijlstra, A.A., Pottasch, S.R., Bignell, C. (1989) A&A S 79, 329 Google Scholar