Quiescent and active flaring periods in SS 433 at 408 MHz

Details Quiescent and active flaring periods in SS 433 at 408 MHz Quiescent and active flaring periods in SS 433 at 408 MHz

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...166..157b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 166, no. 1-2, Sept. 1986, p. 157-166.

Astronomy and Astrophysics

Astronomy

13

Accretion Disks, Radio Sources (Astronomy), Stellar Flares, Radiant Flux Density, Statistical Analysis

Scientific paper

The authors report the flux density measurements of SS433 at 408 MHz over the period April 1980 - March 1984. Quiescent and active flaring periods are distinguished on statistical grounds. The emission is dominated by the so-called quiescent level but in about 20% of the observation time span the source was actively flaring. At least six periods of intense flaring activity were observed, during which the source more than doubled its flux density.

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