Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.202..531h&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 202, Feb. 1983, p. 531-535.
Astronomy and Astrophysics
Astronomy
17
Astronomical Maps, Hydroxyl Emission, Infrared Astronomy, Nebulae, Polarization (Waves), Cosmic Dust, High Resolution, Hydrogen Clouds, Polarimetry
Scientific paper
A high resolution polarization map of OH 0739-14 at 2.2 microns is presented. It is concluded from the polarization data that a scattering mechanism in a bipolar nebula dominates the production of the polarization. The central source of the illumination appears to be scattering by dust grains located at the waist of the 2.2 micron-map, although it is obscured from direct view. The intensity peak at 2.2 microns is one of the polar lobes, while the other polar lobe is much less intense.
Heckert Paul A.
Zeilik Michael II
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