Optical identifications for 3C27, 3C69 and 3C86A

Details Optical identifications for 3C27, 3C69 and 3C86A Optical identifications for 3C27, 3C69 and 3C86A

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...244...37h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 244, no. 1, April 1991, p. 37-42.

Astronomy and Astrophysics

Astronomy

4

Astronomical Photometry, Emission Spectra, Radio Galaxies, Radio Sources (Astronomy), Red Shift, Astrometry, Astronomical Catalogs, Charge Coupled Devices, Signal To Noise Ratios

Scientific paper

Optical identifications have been found for the radio sources 3C27, 3C69 and 3C86A, which are located at low galactic latitudes. For the first two, photometric data have been obtained and redshifts have been determined from low-resolution spectra. In both cases an emission line galaxy is found as the optical counterpart. In the case of 3C27 the galaxy has a broad band magnitude of R = 19.7 and a redshift of z = 0.184, in the case of 3C69 the values are R = 20.9 and z 0.458. The galaxy of 3C86A is similar in appearance to that of 3C27.

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