Non-thermal radio emission of X ray binaries

Details Non-thermal radio emission of X ray binaries Non-thermal radio emission of X ray binaries

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..185p&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 185-196 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

36

Emission Spectra, Nonthermal Radiation, Radio Emission, Stellar Spectra, X Ray Binaries, Extragalactic Radio Sources, Galactic Radiation, Radio Spectra

Scientific paper

A review of the different groups of radio emitting X-ray sources is given. The sources are described along the lines of their X-ray characteristics. Emphasis is placed on the developments in the X-ray/radio correlations in the Z-sources. Some characteristics of the Z-sources are used to determine their distances. The atoll sources, the other group of the persistent bright low mass X-ray binaries, appear to be weaker at radio wavelengths than the Z-sources.

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