Observation of the [O III] λ4363 auroral line in the spectrum of Kaz 163.

Details Observation of the [O III] λ4363 auroral line in the spectrum of Kaz 163. Observation of the [O III] λ4363 auroral line in the spectrum of Kaz 163.

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ap.....43..136k&link_type=abstract

Astrophysics, Vol. 43, No. 2, p. 136 - 140

Astronomy and Astrophysics

Astrophysics

Galactic Nuclei: Electron Densities, Galactic Nuclei: Oxygen Lines, Galactic Nuclei: Line Profiles

Scientific paper

Results of spectroscopic observations of the nucleus of the S component of the galaxy Kaz 163, carried out on the 6-m telescope of the Special Astronomical Observatory in 1982, are presented. The equivalent widths, relative intensities, and half-widths of emission lines were determined. The electron temperature, electron density, and mass of the gaseous component of the nucleus were also determined. The half-widths and equivalent widths varied almost twofold over the time of observations from October 31, 1981, to May 28, 1982. During the same time the intensity of the [O III] λ4363 auroral line increased fairly strongly.

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