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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.
Accretion, Astronomy
Accretion, Astronomy
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 29 | |
popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 10% | |
influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 10% |
views | 75 | |
downloads | 8 |