Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-26T01:42:54.272Z Has data issue: false hasContentIssue false
  • English
  • Français

CCD Spectrophotometry of Planetary Nebulae at Wendelstein Observatory

Published online by Cambridge University Press:  07 August 2017

M. M. Roth ,
R.-P. Kudritzki  and
R. H. Méndez
M. M. Roth
Affiliation:
Universitäts–Sternwarte München, Scheinerstr. 1, 8000 München 80, FRG
R.-P. Kudritzki
Affiliation:
Universitäts–Sternwarte München, Scheinerstr. 1, 8000 München 80, FRG
R. H. Méndez
Affiliation:
Universitäts–Sternwarte München, Scheinerstr. 1, 8000 München 80, FRG

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.

During the past decade the achievements in the theory of stellar atmospheres of hot stars combined with improved spectrograph and detector technology at large telescopes have led to a significantly improved knowledge of PN nuclei properties (see Méndez et al. 1988, Kudritzki and Méndez 1989).

Type
I. The Observational PN Database
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 42
Copyright
Copyright © Kluwer 1993 

References

Gabler, R., Gabler, A., Kudritzki, R.-P., Puls, J., Pauldrach, A., 1989, A&A 226, 162 Google Scholar
Kudritzki, R.P., Méndez, R.H., 1989, in: IAU Symp. 131, ed. Torres-Peimbert, S., Kluwer, p.273 Google Scholar
Méndez, R.H., Kudritzki, R.-P., Herrero, A., Husfeld, D., Groth, H.G., 1988, A&A 190, 113 Google Scholar
Méndez, R.H., Kudritzki, R.-P., Herrero, A., 1992, A&A 260, 329 Google Scholar
Roth, M.M., 1990, in: CCD's in Astronomy , ed Jacoby, G. H., ASP Conf. Series, p.380 Google Scholar