1992
DOI: 10.1086/132958
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The structure of the BAL QSO 1700 + 518

Abstract: ABSTRACT. We present 0.5 arcsec resolution optical images of the low-redshift, bright, broad-absorption-line (BAL) QSO 1700+518. We find a bright arc 2 arcsec 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 structur… Show more

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Cited by 15 publications
(24 citation statements)
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“…Di †use emission surrounding the QSO extends to D5A in deep (3 p \ 25 mag arcsec~2), ground-based V -band images (Hickson & Hutchings 1987 ;Hutchings et al 1992). This structure is presumably associated with the QSO host galaxy, and not the ring galaxy, given the sharpness of the ring edge seen in our images (Fig.…”
Section: T He Qso Hostmentioning
confidence: 99%
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“…Di †use emission surrounding the QSO extends to D5A in deep (3 p \ 25 mag arcsec~2), ground-based V -band images (Hickson & Hutchings 1987 ;Hutchings et al 1992). This structure is presumably associated with the QSO host galaxy, and not the ring galaxy, given the sharpness of the ring edge seen in our images (Fig.…”
Section: T He Qso Hostmentioning
confidence: 99%
“…The double radio source associated with PG 1700]518 Hutchings et al 1992) is apparently not directly associated with the QSO host galaxy or PG 1700]518R, since the position angle di †ers by D50¡.…”
Section: T He Qso Hostmentioning
confidence: 99%
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“…The comparison between the HST and CFHT images of PG 1700+514 shows how powerful AO can be, and bodes well for the use of the technique on 10 m-class telescopes. No obvious relation is found between the near-IR image and the radio map (Hutchings et al 1992). …”
Section: Pg 1700+514mentioning
confidence: 97%