Modeling The Line Strength Of The Optical Jet Lines In Ss 433

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Scientific paper

We present a study of the H-alpha jet emission lines in the spectrum of SS 433. SS 433 is a microquasar which uniquely shows optical emission from the relativistic jets in the system. We use time-series optical spectroscopy to study the line strength of individual ``bullets'' in the jets and model the rate at which the equivalent width decreases. A good understanding of this behavior can lead to more direct comparison of observations to the jet kinematic model, as well as other important system characteristics.

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