Energy spectral distributions and electron temperature of the planetary nebulae

Details Energy spectral distributions and electron temperature of the planetary nebulae Energy spectral distributions and electron temperature of the planetary nebulae

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974crasb.279..227h&link_type=abstract

Academie des Sciences (Paris), Comptes Rendus, Serie B - Sciences Physiques, vol. 279, no. 9, Aug. 26, 1974, p. 227-229. In Fre

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Electron Energy, Planetary Nebulae, Spectral Energy Distribution, Continuous Spectra, Energy Spectra, Point Sources, Stellar Spectrophotometry

Scientific paper

A spectrophotometric method using an oscillating-frame spectrograph was employed to obtain comparisons of the energy spectral distributions between 5000 and 3100 A of four planetary nebulae (NGC 6210, 6543, 6826, and 6572) with those of two standard stars whose spectrophotometric parameters are precisely known. Electron temperatures obtained for these nebulae on the basis of different parameters are then compared.

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