The near-ultraviolet spectrum of Markarian 205

John N. Bahcall, Buell T. Jannuzi, Donald P. Schneider, George F. Hartig, Edward B. Jenkins

Research output: Contribution to journalArticle

19 Scopus citations

Abstract

We report measurements of the absorption and of the emission lines between 1600 and 3200 Å in the spectrum of the nearby AGN Markarian 205 (z = 0.071), which lies at a projected distance of 3 kpc (H0 = 100 km S-1) from the nucleus of the nearby barred spiral galaxy, NGC 4319 (z = 0.0047). The results were obtained using high-resolution (R = 1300) observations with the Faint Object Spectrograph of the Hubble Space Telescope. A total of 15 absorption lines, 13 of which are produced by Galactic gas, and four AGN emission lines are detected. Two of the absorption lines, the Mg II resonant doublet, are produced by gas in the intervening galaxy NGC 4319. This is the first detection of absorption due to intervening gas in this famous quasar-galaxy pair.

Original languageEnglish (US)
Pages (from-to)495-500
Number of pages6
JournalAstrophysical Journal
Volume398
Issue number2
DOIs
StatePublished - Jan 1 1992

    Fingerprint

Keywords

  • Galaxies: active
  • Galaxies: individual (Markarian 205, NGC 4319)
  • Galaxies: seyfert

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Bahcall, J. N., Jannuzi, B. T., Schneider, D. P., Hartig, G. F., & Jenkins, E. B. (1992). The near-ultraviolet spectrum of Markarian 205. Astrophysical Journal, 398(2), 495-500. https://doi.org/10.1086/171872