Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...345..327p&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 345, Oct. 1, 1989, p. 327-338.
Astronomy and Astrophysics
Astronomy
8
Atmospheric Models, Planetary Nebulae, Stellar Atmospheres, Stellar Models, Ultraviolet Spectra, Abundance, Iue, Nonequilibrium Thermodynamics, Stellar Composition, Stellar Temperature, Ultraviolet Astronomy
Scientific paper
Non-LTE hydrogen and helium model atmospheres have been obtained for temperatures and gravities relevant to the central stars of planetary nebulae. Low-resolution and high-resolution observations obtained by the IUE satellite have been used along with optical data to determine Zanstra temperatures of the central stars of NGC 1535, NGC 6210, NGC 7009, IC 418, and IC 4593. Comparison of the observed stellar continuum of these stars with theoretical results allowed further information on the stellar temperature to be derived. The final temperatures are used to calculate accurate stellar parameters.
Cerruti-Sola Monica
Patriarchi Patrizio
Perinotto Mario
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