Hostname: page-component-848d4c4894-tn8tq Total loading time: 0 Render date: 2024-06-14T16:49:48.656Z Has data issue: false hasContentIssue false

Temperatures and Luminosities of Planetary Nebulae Nuclei

Published online by Cambridge University Press:  19 July 2016

Luciana Bianchi
Affiliation:
Osservatorio Astronomico di Torino, Italy
Elsa Recillas
Affiliation:
Instituto de Astronomia, U.N.A.M., Mexico
Michael Grewing
Affiliation:
Astronomisches Institut Tuebingen, West Germany

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.

The location of Planetary Nebulae Nuclei (PNNi) on the H-R diagram is a very important clue to understand the evolution of these objects.

Type
III. Central Stars
Copyright
Copyright © Kluwer 1989 

References

Acker, A., et al., 1982: Publ. Spec, du CDS N.3 (1982)Google Scholar
Bianchi, L., Grewing, M., 1987: A.A., 169, 227 Google Scholar
Bianchi, L., Cerrato, S., Grewing, M., 1987: 169, 227 Google Scholar
Cerrato, S., Bianchi, L., Grewing, M., Baessgen, M., 1987: in “Mass Outflows from stars and galactic nuclei”, Bianchi, and Gilmozzi, eds., Reidel, in pressGoogle Scholar
van der Hucht, K., 1987, private communicationGoogle Scholar
Wesemael, F., 1981: Ap.J. Suppl., 54, 2 Google Scholar
Wesemael, F., et al., 1980: Ap.J. Suppl., 43, 2 Google Scholar