VLBA multi-frequency monitoring of SS433

Details VLBA multi-frequency monitoring of SS433 VLBA multi-frequency monitoring of SS433

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999newar..43..553p&link_type=abstract

New Astronomy Reviews, Volume 43, Issue 8-10, p. 553-557.

Astronomy and Astrophysics

Astronomy

7

Stars: Individual (Ss433), Ism: Jets And Outflows, Radio Continuum: Stars

Scientific paper

We present results of VLBA observations of SS433 at two epochs at 5, 8.4, and 15 GHz. The AU-scale region of the source is resolved and shows the usual quasi-symmetric core-jet structures. But at another epoch, the maps show bright knots ejected a few days before the observation, while the core-complex disappeared. The bright jet components are completely depolarized with fractional polarization less than 0.5%. We also present the first VLBI image of SS433 at 22 GHz.

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