Emission Lines of the Planetary Nebulae (Kondrat'eva, 1979-1985)

Details Emission Lines of the Planetary Nebulae (Kondrat'eva, 1979-1985) Emission Lines of the Planetary Nebulae (Kondrat'eva, 1979-1985)

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat.3203....0k&link_type=abstract

VizieR On-line Data Catalog: III/203. Originally published in: 1985Afz....22..153K; 1979AZh....56..345K

Physics

Nebulae: Planetary, Spectroscopy

Scientific paper

The relative intensities of emission lines in the spectra of 32 planetary nebulae in the 3700-7300Å region are presented. The spectral observations have been carried out using slit spectrograph with three-cascades image-tube, attached to 70-cm reflector (Alma-Ata). The spectral region is 3700-8500Å. The dispersion in the range of 12-200Å/mm. The spectral resolution is 0.8-13Å in dependence on the dispersion. The errors are less than 10% for the bright lines, 10-15% for the moderate lines and 25-50% for the faintest lines. All measured line intensities were normalised to I(Hβ)=100.
(1 data file).

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