The polarization of NGC 1068

Details The polarization of NGC 1068 The polarization of NGC 1068

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234..899b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Oct. 15, 1988, p. 899-917.

Astronomy and Astrophysics

Astronomy

67

Astronomical Spectroscopy, Polarimetry, Seyfert Galaxies, Balmer Series, Forbidden Transitions, H Alpha Line, H Beta Line, High Resolution

Scientific paper

Broad-band polarimetry of NGC 1068 over the wavelength range 0.36 - 4.8
μm is presented, together with high-resolution spectropolarimetry of
the Hβ, [O III] and Hα, [N II] regions of the spectrum. The
authors recognize several different polarization components and conclude
that they can all be accounted for by processes involving dust.

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