Do Galaxies Produce Quasar Absorption Lines? (cycle 0)

Physics

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Hst Proposal Id #1022

Scientific paper

SPECTRA WILL BE OBTAINED WITH THE FOS FOR A NUMBER OF QUASARS SMALL ANGULAR SEPARATION ON THE SKY FROM GALAXIES OR GALAXY V MARK 205, 3C 232, PKS 2020-370, THE GRAVITATIONALLY LENSED QU OBJECTS BEHIND THE BOOTES GALAXY VOID, US 1329 (BEHIND THE BA GALAXY VOID), AND 5C 03.44 (BEHIND M 31). THE SPECTRA WILL BE HYPOTHESIS THAT SOME METALLIC QUASAR ABSORPTION SYSTEMS ARE C LARGE GALAXY HALOS OR DISKS. WF/PC IMAGES WILL ALSO BE OBTAIN GALAXY, 2237+0305, IN ORDER TO LOCATE ACCURATELY THE QUASAR P MEASURE THE SURFACE BRIGHTNESS OF THE INNER REGION OF THE GAL OBSERVATIONS ARE REQUIRED BECAUSE, FOR THE SMALL REDSHIFTS AT WITH LARGE ANGULAR SIZE ARE FOUND, THE RESONANT ATOMIC LINES ULTRAVIOLET.

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