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- W4301014086 abstract "From ROSAT imaging data we have detections and upper limits for a sample of 26 tailed radio sources in clusters of galaxies mostly from the sample of O'Dea & Owen (1985). All sixteen of the detected sources are unresolved in the ROSAT PSPC images. The sources bright enough to perform X-ray spectral analysis have power-law indices similar to BL~Lacs and Seyfert galaxies. We find that there is a highly significant correlation between the core radio flux density and the X-ray flux but only a weak correlation between the total radio flux density and the X-ray flux. The trend is similar to that found in earlier studies of 3C radio galaxies with {sl Einstein} and more recently with ROSAT. The result adds an additional constraint on models for the unification of BL~Lac objects with FR~I radio sources. Also this result indicates that the observed enhanced X-ray emission near tailed sources is more likely to be due to nuclear emission rather than substructure in the extended cluster gas." @default.
- W4301014086 created "2022-10-04" @default.
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- W4301014086 date "1995-08-17" @default.
- W4301014086 modified "2023-09-27" @default.
- W4301014086 title "X-ray properties of head-tail radio sources in clusters of galaxies" @default.
- W4301014086 doi "https://doi.org/10.48550/arxiv.astro-ph/9508077" @default.
- W4301014086 hasPublicationYear "1995" @default.
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