Correlated optical and radio structure in the QSO 1302-102

Details Correlated optical and radio structure in the QSO 1302-102 Correlated optical and radio structure in the QSO 1302-102

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106..642h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 106, no. 700, p. 642-645

Astronomy and Astrophysics

Astronomy

9

Astronomical Maps, Galactic Structure, Quasars, Satellite-Borne Photography, Visible Spectrum, Data Reduction, Flux Density, Hubble Space Telescope, Stellar Luminosity, Very Large Array (Vla)

Scientific paper

We present new optical imaging in two broadband colors of the z = 0.29 bright QSO 1302-102, obtained with the Wide Field Camera (WFC) of the Hubble Space Telescope (HST). We have performed deconvolution on the HST data, previously published Canada-France-Hawaii Telescope (CFHT) HRCam data, and the combined data. The structure and brightness are measured of an extended knot 2.3 arcsec from the QSO, and also of brighter structure in the inner 1 arcsec of the QSO. We compare the optical structure with new and existing maps of the radio structure from the Very Large Array (VLA). The 5 arcsec radio structures lie along the directions of some of the optical components. We discuss the implications.

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