The structure of the BAL QSO 1700 + 518

Details The structure of the BAL QSO 1700 + 518 The structure of the BAL QSO 1700 + 518

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasp..104...62h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 104, Jan. 1992, p. 62-65.

Mathematics

Logic

17

Absorption Spectra, Galactic Nuclei, Line Shape, Quasars, Far Ultraviolet Radiation, Red Shift, Ultraviolet Spectra

Scientific paper

The paper presents 0.5-arcsec-resolution optical images of the low-redshift, bright, broad-absorption-line QSO 1700 + 518. A bright arc 2 arcsec is found to the NE of the nucleus which is redder than the surrounding host galaxy. There is also a faint radial structure to the SE, which is aligned with the core radio structure. The principal radio structure is a slightly resolved component coincident with the optical nucleus and an unresolved lobe 1 arcsec to the W which has no corresponding optical structure. The morphological and other properties of the QSO are discussed.

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