Monitoring of very rapid changes in the optical spectrum of SS 433 in May/June 1987

Details Monitoring of very rapid changes in the optical spectrum of SS 433 in May/June 1987 Monitoring of very rapid changes in the optical spectrum of SS 433 in May/June 1987

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...270..204v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 270, no. 1-2, p. 204-222.

Astronomy and Astrophysics

Astronomy

33

Eclipsing Binary Stars, H Lines, Line Shape, Radio Jets (Astronomy), Visible Spectrum, Balmer Series, Data Bases

Scientific paper

The evolution of the moving emission lines from the jets of SS 433 was studied on an hourly timescale for several weeks in May/June 1987; the emission lines' properties are describable in terms of discrete line components whose approaching and receding properties are the same after compensation for orientation effects. A need is identified for models that can explain the contrast between the clumpiness of the jets, as seen in optical line emission, and the more continuous outflow suggested by X-ray and radio emission.

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