A dynamical model for the radio outbursts of Cygnus X-3

Details A dynamical model for the radio outbursts of Cygnus X-3 A dynamical model for the radio outbursts of Cygnus X-3

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...208..863w&link_type=abstract

Astrophysical Journal, vol. 208, Sept. 15, 1976, pt. 1, p. 863-872.

Astronomy and Astrophysics

Astronomy

5

Astronomical Models, Dynamic Models, Radio Bursts, Radio Sources (Astronomy), X Ray Sources, Decay Rates, Radiant Flux Density, Stellar Evolution, X Ray Spectra

Scientific paper

The observed exponential decay of the first Cygnus X-3 radio burst is explained by an expanding cloud model which has an exponentially increasing radius. The model also predicts an exponential rise, which is actually observed, and an exponentially decaying emission measure, as found by Gregory and Seaquist (1974). It is shown that the temperature of the absorbing plasma is not constant, and this can explain the anomalously low peaks at high frequencies. A dynamical history is presented which predicts the observed exponential stage and subsequent evolution to a stable power law.

Affiliated with

Also associated with

No associations

Rating

A dynamical model for the radio outbursts of Cygnus X-3 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A dynamical model for the radio outbursts of Cygnus X-3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A dynamical model for the radio outbursts of Cygnus X-3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1413456