The determination of the temperatures of planetary nebulae nuclei from the relative He I/H-beta and He II/H-beta line intensities

Details The determination of the temperatures of planetary nebulae nuclei from the relative He I/H-beta and He II/H-beta line intensities The determination of the temperatures of planetary nebulae nuclei from the relative He I/H-beta and He II/H-beta line intensities

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..724g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, July-Aug. 1987, p. 724-733. In Russian.

Statistics

Computation

3

Computational Astrophysics, Gas Temperature, H Beta Line, Helium Ions, Planetary Nebulae, Spectral Energy Distribution

Scientific paper

The results of determination of planetary nebulae nuclei temperatures are presented. The Zanstra method modified for the He admixture was used. Analytical forms and graphic representations convenient for practical temperature determination are presented. T* values for 51 planetary nebulae nuclei are found. These T* values agree with the temperatures found by the energy balance method. Validity of nuclei temperature determination by this method is discussed.

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