Hostname: page-component-7bb8b95d7b-wpx69 Total loading time: 0 Render date: 2024-09-12T12:15:48.433Z Has data issue: false hasContentIssue false
  • English
  • Français

Correlation between N/O nebular ratio and central star mass: distances to Galactic PN

Published online by Cambridge University Press:  25 May 2016

J. O. Cazetta  and
W. J. Maciel
J. O. Cazetta
Affiliation:
Instituto Astronômico e Geofísico da USP, São Paulo, Brazil
W. J. Maciel
Affiliation:
Instituto Astronômico e Geofísico da USP, São Paulo, Brazil

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.

In the planetary nebulae (PNe) studies, their distance determination remains a confusing issue. The statistical distance scales cannot be regarded as reliable, and there are few PNe with individual distance determinations. In this work, we present a distance scale based on the method of individual distance determination by Méndez et al. (1988, A&A 190, 113).

Type
II. Distances to Galactic Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 46
Copyright
Copyright © Kluwer 1997