A bright flaring state of SS433

Details A bright flaring state of SS433 A bright flaring state of SS433

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..960....1t&link_type=abstract

The Astronomer's Telegram, #960

Astronomy and Astrophysics

Astronomy

Radio, Millimeter, Optical, X-Ray, Request For Observations, Binaries, Black Holes, Transients

Scientific paper

We report that the super-critical microquasar SS433 is the flaring state at radio waves and the optical band and would request for followup observations at all frequencies. In the monitoring program of microquasars with the RATAN-600 radio telescope (Trushkin et al., astro-ph/0611550), the flux densities at 1-22 GHz increased from a quiet optically thin synchrotron spectrum: S_nu[Jy] = 1.05*nu^-0.54[GHz] on 2006 Dec 6.48 (UT) to flaring one: S_nu[Jy] = 2.90*nu^-0.43[GHz] on 2006 Dec 8.47 (MJD54077.47) for the total range of 1-22 GHz.

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