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- W2899582125 abstract "We investigate the role of environment on radio galaxy properties by constructing a sample of large (≳100 kpc), nearby (|$z$| < 0.3) radio sources identified as part of the Radio Galaxy Zoo citizen science project. Our sample consists of 16 Fanaroff-Riley Type II (FR-II) sources, 6 FR-I sources, and 1 source with a hybrid morphology. FR-I sources appear to be hosted by more massive galaxies, consistent with previous studies. In the FR-II sample, we compare the degree of asymmetry in radio lobe properties to asymmetry in the radio source environment, quantified through optical galaxy clustering. We find that the length of radio lobes in FR-II sources is anticorrelated with both galaxy clustering and lobe luminosity. These results are in quantitative agreement with predictions from radio source dynamical models and suggest that galaxy clustering provides a useful proxy for the ambient gas density distribution encountered by the radio lobes." @default.
- W2899582125 created "2018-11-16" @default.
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- W2899582125 date "2018-11-13" @default.
- W2899582125 modified "2023-10-06" @default.
- W2899582125 title "Radio Galaxy Zoo: observational evidence for environment as the cause of radio source asymmetry" @default.
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- W2899582125 doi "https://doi.org/10.1093/mnras/sty3070" @default.
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