Hot central stars in planetary nebulae

Details Hot central stars in planetary nebulae Hot central stars in planetary nebulae

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..329m&link_type=abstract

In ESA Fourth European IUE Conf. p 329-331 (SEE N84-35135 24-88)

Astronomy and Astrophysics

Astronomy

1

Hot Stars, Planetary Nebulae, Spectrum Analysis, Stellar Radiation, Stellar Temperature, Continuous Radiation, Iue, Spaceborne Astronomy, Stellar Spectra, Ultraviolet Spectra

Scientific paper

The Zanstra temperature is determined for five hot stars using IUE
spectra. The ultraviolet part of the spectrum is much more favourable
than the visual region for such a determination because the stellar
continuum flux density is much stronger relative to the nebular
continuum in the ultraviolet.

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