Study of the nuclei of planetary nebulae at UV wavelengths

Details Study of the nuclei of planetary nebulae at UV wavelengths Study of the nuclei of planetary nebulae at UV wavelengths

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b.173b&link_type=abstract

In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 173-176 (SEE N89

Astronomy and Astrophysics

Astronomy

2

Iue, Planetary Nebulae, Spaceborne Astronomy, Stellar Spectra, Ultraviolet Astronomy, Ultraviolet Spectra, Stellar Atmospheres, Stellar Luminosity, Stellar Models, Stellar Radiation, Stellar Temperature

Scientific paper

The T eff of planetary nebulae nuclei were determined by comparison of the stellar continuum flux with black-body or model atmospheres, using IUE low resolution spectra and data from the literature at other wavelengths. Results are compared with determinations based on other methods. To determine the luminosity, distances were taken from the literature or rederived, and the value of the stellar radius was obtained from the model fit to the absolute UV flux.

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