Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-14T20:16:56.455Z Has data issue: false hasContentIssue false
  • English
  • Français

Interstellar Extinction of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

G. Stasinska ,
R. Tylenda ,
A. Acker  and
B. Stenholm
G. Stasinska
Affiliation:
1)DAEC, Observatoire de Paris-Meudon, France
R. Tylenda
Affiliation:
1)DAEC, Observatoire de Paris-Meudon, France 2)Observatoire de Strasbourg, France 3)Copernicus Astronomical Center, Torun, Poland
A. Acker
Affiliation:
2)Observatoire de Strasbourg, France
B. Stenholm
Affiliation:
4)Lund Observatory, Sweden

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.

We have compared the extinction of planetary nebulae (PN) as derived from the Balmer decrement and from the ratio of radio to Hβ fluxes.

Type
III. Highlights on the Nebulae
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 177
Copyright
Copyright © Kluwer 1993