Very high resolution observations of the nearby quasar 0241+622

Details Very high resolution observations of the nearby quasar 0241+622 Very high resolution observations of the nearby quasar 0241+622

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....76l..21g&link_type=abstract

Astronomy and Astrophysics, vol. 76, no. 3, July 1979, p. L21, L22.

Astronomy and Astrophysics

Astronomy

12

High Resolution, Quasars, Very Long Base Interferometry, X Ray Sources, Interstellar Extinction, Radiant Flux Density, Radio Astronomy

Scientific paper

Very high-resolution observations of the nearby quasar 0241+622 have been made. The measured angular size of 0.00055 + or - 0.00010 arcsec corresponds to a linear size of 0.63 + or - 0.11 parsecs and appears to be dominated by the effect of interstellar scattering, so the true size may be much smaller. No evidence is found for high-frequency flux-density variations of the source over a six-month interval. In comparison with other compact radio sources, 0241+622 is one of the strongest emitters per unit volume.

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