High dispersion EUV observations of planetary nebulae

Details High dispersion EUV observations of planetary nebulae High dispersion EUV observations of planetary nebulae

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.157..191k&link_type=abstract

The second European International Ultraviolet Explorer (IUE) Conference, held 26-28 March 1980 in Tübingen, West Germany. Edited

Astronomy and Astrophysics

Astronomy

5

Absorption Spectra, Emission Spectra, Iue, Planetary Nebulae, Ultraviolet Astronomy, Carbon, Continuous Spectra, Helium, Interstellar Matter, Subdwarf Stars

Scientific paper

The three high excitation planetary nebulae NGC 3242, NGC 7009 and NGC 6210 were observed in the short wavelength range with high resolution. The most prominent emission lines are the He (II) 1640 and C (III) 1909 A lines. The C (IV) 1550 lines of NGC 3242 and NGC 7009 are in emission, whereas in NGC 6210 they are in absorption. This suggests that the central star of NGC 6210 is a subdwarf O.

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