Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Spectrophotometry of the Seyfert galaxy NGC 4593

Journal Article · · Publ. Astron. Soc. Pac.; (United States)
DOI:https://doi.org/10.1086/130580· OSTI ID:5129097

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.

Research Organization:
Michigan Univ., Ann Arbor
OSTI ID:
5129097
Journal Information:
Publ. Astron. Soc. Pac.; (United States), Journal Name: Publ. Astron. Soc. Pac.; (United States) Vol. 91; ISSN PASPA
Country of Publication:
United States
Language:
English

Similar Records

Spectrophotometry of the nucleus of the Seyfert Galaxy NGC 7469
Journal Article · Fri Jul 01 00:00:00 EDT 1988 · Astrophysics (Engl. Transl.); (United States) · OSTI ID:6321566

Spectrophotometric investigation of the galaxy NGC 3353
Journal Article · Mon Sep 01 00:00:00 EDT 1986 · Astrophysics (Engl. Transl.); (United States) · OSTI ID:6955470

Extended ionized gas in the Seyfert 2 galaxy NGC 4388
Journal Article · Thu Sep 01 00:00:00 EDT 1988 · Astrophys. J.; (United States) · OSTI ID:6862200