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

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

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.0314l&link_type=abstract

American Astronomical Society, AAS Meeting #211, #03.14; Bulletin of the American Astronomical Society, Vol. 39, p.725

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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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