Structure of the Haro 6-5 complex

Details Structure of the Haro 6-5 complex Structure of the Haro 6-5 complex

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.223..867g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 223, Dec. 15, 1986, p. 867-875. SERC-supported research

Astronomy and Astrophysics

Astronomy

13

Emission Spectra, Herbig-Haro Objects, Linear Polarization, Stellar Winds, Optical Emission Spectroscopy, Polarimetry, T Tauri Stars

Scientific paper

The authors present an imaging polarization study of the Haro 6-5 complex, including its emission-line jet feature. They identify the sources of illumination and suggest a geometrical interpretation for the system. In the R waveband the emission-line jet is linearly polarized at a level of 18±2% at PA 147±8°, implying that it is a reflection phenomenon. The authors discuss the implications of this observation.

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