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        Near-IR Spectropolarimetry of NGC 1088

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        901680.pdf (PDF, 154Kb)
        Author
        Young, S.
        Hough, J.
        Bailey, J.
        Axon, D.J.
        Ward, M.J.
        Attention
        2299/1550
        Abstract
        The current unified model of Seyfert galaxies, as proposed by Antonucci and Miller (1985), has most, if not all, Seyfert 2 galaxies hosting a Seyfert 1 type nucleus in their cores. The broad lines from the type 1 nucleus can be scattered and be seen in the polarized flux spectrum, provided the geometry is correct. Whether the mechanism is electron or dust scattering has been a question of some debate. Since dust would normally have a low scattering efficiency in the infrared, near-IR spectropolarimetry should help in determing the nature of the scatterers. To this end we present the first near-IR spectropolarimetry of NGC 1068 a "Seyfert 2" galaxy in which polarized broad lines have been observed at optical wavelengths.
        Publication date
        1994
        Published in
        In: Procs of The First Stromlo Symposium: The Physics of Active Galaxies. ASP Conference Series 54
        Other links
        http://hdl.handle.net/2299/1550
        Relations
        School of Physics, Astronomy and Mathematics
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