High-resolution imaging of QSO 2305 + 187 (= 4C 18.68)

Details High-resolution imaging of QSO 2305 + 187 (= 4C 18.68) High-resolution imaging of QSO 2305 + 187 (= 4C 18.68)

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasp..104...66h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 104, Jan. 1992, p. 66-70.

Astronomy and Astrophysics

Astronomy

4

Hubble Space Telescope, Image Resolution, Interacting Galaxies, Quasars, Red Shift, Emission Spectra, High Resolution, Line Spectra

Scientific paper

Optical imaging of QSO 2305 + 187 with resolution ranging from 0.1 to 1.0 arcsec in continuum and line emission is presented. The data are from FOCAM and the HR Cam of the Canada-France-Hawaii Telescope, and the Wide Field Camera of the Hubble Space Telescope. These are compared with previously published optical and radio images. The QSO host galaxy has the basic properties of an elliptical, but has significant irregularities, and tidal tails which indicate an ongoing gravitational interaction with a close companion.

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