Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-23T20:28:00.705Z Has data issue: false hasContentIssue false
  • English
  • Français

HR Diagram of Evolved Stars

Published online by Cambridge University Press:  30 March 2016

D. Schönberner
D. Schönberner*
Affiliation:
Institut für Theoretische Physik & Sternwarte Universität Kiel2300 KielGermany

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.

A short review is presented on the various methods to construct the HR diagram for central stars of planetary nebulae (CPN).

Type
Joint Commission Meetings
Information
Highlights of Astronomy , Volume 9: Highlights of Astronomy. As presented at the XXIst General Assembly of the IAU, 1991 , 1992 , pp. 635 - 637
Copyright
Copyright © Kluwer 1992

References

Aller, L.H., Keyes, C.D., Moran, S.P., Gull, T.P., Michalitsianos, A.G., Stecher, T.P., 1987, Astrophys. J. 320, 101 Google Scholar
Ambartsumyan, V.A., 1932, Pulkovo Obs. Circ. No. 4, 8 Google Scholar
Harman, R.J., Seaton, M.J., 1966, Mon. Not. R. astr. Soc. 132, 101 Google Scholar
Henry, R.B., Liebert, J., Boroson, T.A., 1989, Astrophys. J. 339, 872 CrossRefGoogle Scholar
Jacoby, G.H., Kaler, J.B., 1989, Astron. J. 98, 1662Google Scholar
Kaler, J.B., Jacoby, G.H., 1988, Astrophys. J. 345, 101 Google Scholar
Méndez, R., 1991 in Stellar Atmospheres-beyond classical models, eds. Crivellari, , Hubeny, , Hummer, (Kluwer) p. 331 Google Scholar
Monk, D.J., Barlow, M.J., Clegg, R.E.S., 1987, LAU Symp. 131, Planetary Nebulae, p. 355 Google Scholar
Schönberner, D., Tylenda, R., 1990, Astron. Astrophys. 234, 101 Google Scholar
Tylenda, R., Stasinska, G., Acker, A., Stenholm, B., 1991, Astron. Astrophys.Google Scholar