EDP Sciences
Free Access
Volume 404, Number 2, June III 2003
Page(s) 505 - 511
Section Galactic structure and dynamics
DOI https://doi.org/10.1051/0004-6361:20030558
Published online 02 June 2003

A&A 404, 505-511 (2003)
DOI: 10.1051/0004-6361:20030558

Spectropolarimetry of the borderline Seyfert 1 galaxy ESO 323-G077

H. M. Schmid1, I. Appenzeller2 and U. Burch1

1  Institut für Astronomie, ETH Zentrum, 8092 Zürich, Switzerland
2  Landessternwarte Heidelberg-Königstuhl, 69117 Heidelberg, Germany

(Received 19 December 2002 / Accepted 31 March 2003 )

We report the detection of high linear polarization in the bright Seyfert 1 galaxy ESO 323-G077 . Based on optical spectropolarimetry with FORS1 at the VLT we find a continuum polarization which ranges from 2.2% at 8300 Å to 7.5% at 3600 Å. Similar amounts of linear polarization are found for the broad emission lines, while the narrow lines are not polarized. The position angle of the polarization ( $\theta=84^\circ$) is independent of the wavelength and found to be perpendicular to the orientation of the extended [O III] emission cone of this galaxy. Within the standard model of Seyfert nuclei the observations can be well understood assuming that this AGN is observed at an inclination angle where the nucleus is partially obscured and seen mainly indirectly in the light scattered by dust clouds within or above the torus and the illuminated inner edge of the dust torus itself. Hence we conclude that ESO 323-G077 is a borderline Seyfert 1 galaxy which can provide important information on the geometric properties of active nuclei.

Key words: galaxies: active -- galaxies: Seyfert -- galaxies: individual: ESO 323-G077 -- polarization -- scattering

Offprint request: H. M. Schmid, schmid@astro.phys.ethz.ch

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© ESO 2003

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