Relativistic jets in stellar X-ray sources.

Details Relativistic jets in stellar X-ray sources. Relativistic jets in stellar X-ray sources.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..111m&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 111 - 114

Astronomy and Astrophysics

Astrophysics

2

X-Ray Binaries: Relativistic Jets

Scientific paper

The authors review the observational properties of the two galactic superluminal sources GRS 1915+105 and GRO J1655-40, and compare them with SS433 and other stellar X-ray sources of relativistic jets. Hard X-ray transients produce sporadic ejections of discrete plasma clouds at speeds close to the velocity of light. Persistent sources of hard X-rays produce more continuous flows of relativistic particles, and are usually associated with faint, mildly variable radio cores at the center of double-sided synchrotron radio jets that stretch over several light-years.

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