Spectroscopy of radio sources from the third Bologna survey

Details Spectroscopy of radio sources from the third Bologna survey Spectroscopy of radio sources from the third Bologna survey

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..113d&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, Feb. 1990, p. 113-116. Research supported by the A

Astronomy and Astrophysics

Astronomy

13

Astronomical Spectroscopy, Quasars, Radio Sources (Astronomy), Sky Surveys (Astronomy), Active Galactic Nuclei, Charge Coupled Devices, Emission Spectra, Interacting Galaxies, Red Shift

Scientific paper

Long-slit CCD spectroscopy is presented for 11 optical candidates for selected radio sources from the third Bologna survey (B3). One object (0141 + 398) is a probable misidentification, a foreground star. The remaining objects are a mixture of quasars and active galaxies, ranging in redshift from 0.11 to 0.85. B3 0219 + 443 is a steep-spectrum quasar. B3 1141 + 374 is identified with an interacting galaxy pair, with the southern component harboring an active nucleus.

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