Relativistic Jets in SS 433
- 15 January 1982
- journal article
- research article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 215 (4530) , 247-252
- https://doi.org/10.1126/science.215.4530.247
Abstract
A variety of recent optical, radio, and x-ray observation have confirmed the hypothesis that the peculiar star SS 433 is ejecting two narrow, opposed, highly collimated jets of matter at one-quarter the speed of light. This unique behavior is probably driven by mass exchange between a relatively normal star and a compact companion, either a neutron star or a black hole. However, numerous details regarding the energetics, radiation, acceleration, and collimation of the jets remain to be understood. This phenomenon may well be a miniature example of similar collimated ejection of gas by active extragalactic objects such as quasars and radio galaxies.Keywords
This publication has 35 references indexed in Scilit:
- SUMMARY OF THE WORKSHIP ON SS 433Annals of the New York Academy of Sciences, 1981
- Periodic changes in the compact radio structure of SS 433The Astrophysical Journal, 1981
- Short-period variations in the moving line spectrum of SS 433The Astronomical Journal, 1981
- An analysis of the proper motions of SS 433 radio jetsThe Astrophysical Journal, 1981
- Changes in orientation and appearance of the 100 m arc s radio structure in SS433Nature, 1981
- SS 433 as a prototype of astrophysical jetsThe Astrophysical Journal, 1980
- Diffuse X-ray emission from the jets of SS433Nature, 1980
- Disk-driven precession in SS 433The Astrophysical Journal, 1980
- Enormous periodic Doppler shifts in SS 433The Astrophysical Journal, 1979
- The bizarre spectrum of SS 433The Astrophysical Journal, 1979