An offset seyfert 2 nucleus in the minor merger system ngc 3341

Aaron J. Barth, Misty C. Bentz, Jenny E. Greene, Luis C. Ho

Research output: Contribution to journalArticle

41 Scopus citations

Abstract

We present the discovery of a triplet of emission-line nuclei in the disturbed disk galaxy NGC 3341, based on archival data from the Sloan Digital Sky Survey and new observations from the Keck Observatory. This galaxy contains two offset nuclei within or projected against its disk, at projected distances of 5.1 and 8.4 kpc from its primary nucleus and at radial velocity separation of less than 200 km s-1 from the primary. These appear to be either dwarf ellipticals or the bulges of low-mass spirals whose disks have already been stripped off while merging into the primary galaxy. The inner offset nucleus has a Seyfert 2 spectrum and a stellar velocity dispersion of 70 ± 7 km s-1. The outer offset nucleus has very weak emission lines consistent with a LINER classification, and the primary nucleus has an emission-line spectrum close to the boundary between LINER/H n composite systems and H II nuclei; both may contain accreting massive black holes, but the optical classifications alone are ambiguous. The detection of an offset active nucleus in NGC 3341 provides a strong suggestion that black hole accretion episodes during minor mergers can be triggered in the nuclei of dwarf secondary galaxies as well as in the primary.

Original languageEnglish (US)
Pages (from-to)L119-L122
JournalAstrophysical Journal
Volume683
Issue number2 PART 2
DOIs
StatePublished - Jan 1 2008

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Galaxies: Active
  • Galaxies: Individual (NGC 3341)
  • Galaxies: Interactions
  • Galaxies: Nuclei
  • Galaxies: Seyfert

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