Relativistic Jets from Black-Hole X-ray Transients and Binaries

Details Relativistic Jets from Black-Hole X-ray Transients and Binaries Relativistic Jets from Black-Hole X-ray Transients and Binaries

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..apr..h801h&link_type=abstract

American Physical Society, APS/AAPT Joint April Meeting, April 18-21, 1998 Columbus, Ohio, abstract #H8.01

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Radio imaging of highly relativistic, and sometimes superluminal, radio jets from X-ray transients like GRS 1915+105 and GRO J1655-40 and X-ray binaries like Cyg X-3 and SS433 is the main indicator of jet outflows from accretion disks around black holes, and possibly other compact objects in our Galaxy. The properties of these and other galactic radio jet sources will be reviewed, and the relation between X-ray and radio events will be discussed. The extent to which relativistic effects affect the observations will be part of the discussion.

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