J. Heidt 1,
K. Nilsson 2,
J.W. Fried 3,
L.O. Takalo 2 and
A. Sillanpää 2
Received 4 May 1999 / Accepted 11 May 1999
We present subarcsecond resolution imaging and spectroscopy of the BL Lac object 1ES 1741+196 and neighboring galaxies. Based on 2-dimensional modelling, the host galaxy of 1ES 1741+196 is a very bright and large elliptical galaxy ( = -24.85, = 51.2 kpc) whose overall luminosity distribution deviates significantly from a de Vaucouleurs profile. It is one of the most luminous and largest BL Lac host galaxies known.
Closeby to 1ES 1741+196 we found two companion galaxies at the same redshift as the BL Lac itself. They are at projected distances of 7.2 and 25.2 kpc, respectively. The closer companion galaxy can be best modelled by a Sa-type galaxy, whereas the more distant companion galaxy is an elliptical. This is supported by their spectra. We detected a tidal tail emerging from the closer companion galaxy which is possibly connected with the more distant galaxy. Its surface brightness increases towards the closer companion galaxy, which suggests that material has been released from that galaxy due to tidal forces.
The flat luminosity profile ( = 0.15), high ellipticity ( = 0.35) of the host galaxy of 1ES 1741+196 as well as its position angle along the impact parameter to the neighboring galaxies can be the result of tidal interaction. 1ES 1741+196 may be a BL Lac object in a triplet of interacting galaxies.
Key words: galaxies: photometry galaxies: interactions galaxies: BL Lacertae objects: individual: 1ES 1741+196 galaxies: active methods: data analysis
* Based on observations made with the Nordic Optical Telescope, operated on the island of La Palma, jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Institute de Astrofisica de Canarias.
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© European Southern Observatory (ESO) 1999
Online publication: July 16, 1999