Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-26T01:15:20.392Z Has data issue: false hasContentIssue false
  • English
  • Français

Planetary Nebulae: A Probe of the Galaxies Evolution up to the Hubble Time

Published online by Cambridge University Press:  01 August 2006

A. F. Kholtygin  and
Yu. V. Milanova
A. F. Kholtygin
Affiliation:
Astronomical Institute of Saint-Petersburg, University, Russia email: [email protected]
Yu. V. Milanova
Affiliation:
Astronomical Institute of Saint-Petersburg, University, Russia email: [email protected]
Rights & Permissions [Opens in a new window]

Extract

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.

Chemical evolution of the galactic and extragalactic planetary nebulae (PNe) system beginning from the early age of the Galaxy is investigated. We determine the radial and vertical abundance gradients for C, N, O, Ne, Ar, Cl and S in a dependence on mass and age of the progenitor stars of the nebula. In the Table 1 we compare the galactic abundance gradients for O and Ne for our and neigbour galaxies.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 324
Copyright
Copyright © International Astronomical Union 2007

References

Cedrés, B., Urbaneja, M.A., & Cepa, J. 2004, A&A 422, 511.Google Scholar
Crocket, K.C., Newton, R.J., Bottrell, S.H., & Wignall, P.B. 2006, ApJ 637, 741.CrossRefGoogle Scholar
Garnett, D.R. & Shields, G.A. 1987, ApJ 317, 82.CrossRefGoogle Scholar
Garnett, D.R., Shields, G.A., Skillman, E.D., Sagan, S.P., & Dufour, R.J. 1997, ApJ 489, 63.CrossRefGoogle Scholar
van den Hoek, L.B., & Groenewegen, M.A.T. 1997, A&A Suppl. Ser. 123, 305.CrossRefGoogle Scholar