Investigations of the nebula S 216 at decameter wavelengths

Details Investigations of the nebula S 216 at decameter wavelengths Investigations of the nebula S 216 at decameter wavelengths

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...11a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, Mar.-Apr. 1987, p. 11-14. In Russian.

Astronomy and Astrophysics

Astronomy

2

Astronomical Spectroscopy, Decametric Waves, Planetary Nebulae, Radio Spectra, Electron Density (Concentration), Electron Energy, Mass Distribution

Scientific paper

The thermal nature of radiation from nebula S 216 is established on the
basis of measurements performed at decameter wavelengths. If S 216 is a
planetary nebula, its electron temperature is equal to 8000 + or - 2500
K, its electron density is 5.5 + or - 2.5/cu cm, and its mass is 0.9
solar mass.

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