MK 380 - A Seyfert galaxy at Z = 0.475

Details MK 380 - A Seyfert galaxy at Z = 0.475 MK 380 - A Seyfert galaxy at Z = 0.475

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...168...62g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 168, no. 1-2, Nov. 1986, p. 62-64.

Astronomy and Astrophysics

Astrophysics

Astronomical Spectroscopy, Galactic Nuclei, Quasars, Red Shift, Seyfert Galaxies, Balmer Series, Continuous Spectra, Emission Spectra, Iron, Luminosity, Visible Spectrum

Scientific paper

Mk 380 is classified as a high redshift QSO (z = 2.737) in the catalog of Véron and Véron (1985). New spectrophotometric observations yield instead z = 0.475 and a luminosity both in the lines and the continuum comparable to that of the galaxy Fairall 9. Mk 380 is therefore the most distant genuine Seyfert I nucleus observed to date. The authors also draw attention to its strong Fe II line spectrum and hard optical continuum.

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