Spectrophotometry of the Seyfert galaxy NGC 4593

Details Spectrophotometry of the Seyfert galaxy NGC 4593 Spectrophotometry of the Seyfert galaxy NGC 4593

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..746m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, Dec. 1979-Jan. 1980, p. 746-748. Research supported by the Universi

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24

Astronomical Spectroscopy, Barred Galaxies, Seyfert Galaxies, Spectrophotometry, Balmer Series, Emission Spectra, H Lines, Telescopes

Scientific paper

Spectrophotometry of the bright class 1 Seyfert galaxy NGC 4593 is presented. The emission-line characteristics are briefly discussed and compared with those of other Seyfert galaxies. The measured hydrogen Balmer-line ratios are reasonably consistent with expected recombination values, and the emission intensities of Fe II, He I 5876, and forbidden O III 4363 relative to other lines are stronger than average in NGC 4593.

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