Uv Imaging of the Nearby QSO 2130+099 Host Galaxy

Details Uv Imaging of the Nearby QSO 2130+099 Host Galaxy Uv Imaging of the Nearby QSO 2130+099 Host Galaxy

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5298h&link_type=abstract

HST Proposal ID #5298

Physics

Hst Proposal Id #5298 Quasars &Amp, Agn Quasar Absorption

Scientific paper

The host galaxy of QSO 2130+099 is suspected to be a barred spiral (Hickson & Hutchings 1987, Heap 1986). We will use the unique imaging capabilities of the GHRS to map the nucleus of QSO 2130+099 in UV (1200- 3200A) light. These observations will (1) demonstrate that the GHRS' imaging capabilites have been recovered by COSTAR, and (2) provide the first high-resolution optical map of the nucleus/inner host galaxy of a quasar. THIS IS PART OF HEAP'S CYCLE-4 GTO PROGRAM.

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