Article
Article
SS 433
Article By:
Migliari, Simone Department of Astronomy and Meteorology, University of Barcelona, Barcelona, Spain.
Last reviewed:June 2020
DOI:https://doi.org/10.1036/1097-8542.649950
- Discovery
- Geometry of the jets
- Electromagnetic radiation from jets
- Binary system
- Equatorial outflow
- Related Primary Literature
- Additional Reading
A binary star system in the Milky Way Galaxy consisting of a compact object, possibly a black hole, that accretes matter in the form of a disk from an early-type companion star. The most remarkable feature of the system is the presence of bipolar narrow outflows of matter, jets, with a velocity of 26% the speed of light, whose ejection axes change with time. See also: Black hole; Neutron star
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