Physical conditions in the nuclei of emission-line galaxies

Details Physical conditions in the nuclei of emission-line galaxies Physical conditions in the nuclei of emission-line galaxies

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..267p&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, June 1979, p. 267-270.) Soviet Astronomy Letters, vol. 5, May-June 1979, p. 141-144.

Astronomy and Astrophysics

Astronomy

4

Astronomical Spectroscopy, Emission Spectra, Galactic Nuclei, Spectral Line Width, Spectrophotometry, Abundance, Electron Density (Concentration), H Alpha Line, Hydrogen Ions, Nitrogen Ions, Oxygen Spectra

Scientific paper

Equivalent widths and relative intensities of emission lines in the red
spectral region have been determined for 49 galaxies exhibiting
emission, on the basis of spectrograms obtained with the 125-cm
reflector of the Crimean station, Shternberg Astronomical Institute. The
electron density and the abundance of several ions are estimated.

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