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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

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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