Published December 1979 | Version v1
Journal article

Spectrophotometry of the Seyfert galaxy NGC 4593

  • 1. Michigan Univ., Ann Arbor

Description

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

Additional details

Publishing Information

Journal Title
Publ. Astron. Soc. Pac.
Journal Volume
91
Series
Publ. Astron. Soc. Pac.
Journal Page Range
746-748
ISSN
0004-6280

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
14726390
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BALMER LINES; EMISSION SPECTRA; SEYFERT GALAXIES; SPECTROPHOTOMETRY; SPIRAL CONFIGURATION; TELESCOPES
Descriptors DEC
CONFIGURATION; GALAXIES; SPECTRA