Radio/X-Ray Correlation Database For X-Ray Binaries
收藏资源简介:
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.



