RATAN-600 and EVN observations of quasar 0642+449

Details RATAN-600 and EVN observations of quasar 0642+449 RATAN-600 and EVN observations of quasar 0642+449

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3...21v&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 21-25

Computer Science

1

Scientific paper

Observational results for the high redshift quasar OH 471 obtained by means of RATAN-600 in March and May 1998 at 0.96, 2.3, 3.9, 7.7, 11.2, 21.7 GHz are presented. The radio spectrum of source has a peak at about 20 GHz. We present 1.6 GHz EVN observations of OH 471. Our VLBI data showed that 0642+449 has an extended structure like core-jet. The jet was elongated for about 5 mas to the East. The flux density of the core component was 0.328 Jy.

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