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Published May 24, 2018 | Version v0.1
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Radio/X-ray correlation database for X-ray binaries

  • 1. Curtin University
  • 2. Michigan State University
  • 3. University of Alberta
  • 4. University of Oxford

Description

The radio-X-ray correlation in accretion neutron stars and black holes has been discussed in detail in the literature. BH X-ray binaries (XRBs) show compact partially self-absorbed jet emission in quiescence and in the hard state during outbursts, making them brighter in radio compared to NS LMXBs with similar X-ray luminosities. Since, there have been numerous efforts at further exploring and understanding this correlation. Numerous sources (both known and newly identified) have been observed in radio and X-rays. Here, we have compiled a collection of these measurements from the literature and we actively add new measurements as we notice new publications. This package contains a catalog of radio and X-ray observations of Galactic X-ray binaries as reported in literature. 

 

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