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- W2079968761 abstract "Ultraviolet IUE and soft X-ray EXOSAT observations are presented for the quasar 3C 263 which reveal the low-energy part of the ionizing continuum and allow the high-energy tail to be strongly constrained. The ionizing spectrum confirms that the pressure of the extra-nuclear emission-line gas around the quasar is greater than 10 6 cm −3 K at ∼ 20 kpc. The high pressure of the emission-line gas is interpreted as due to confinement by dense, cooling intracluster gas, qualitatively similar, but of a greater magnitude, to that found in nearby clusters of galaxies. The minimum equipartition pressure of the resolved radio emission from the quasar is in agreement with the pressure profile inferred from the optical data." @default.
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- W2079968761 date "1991-01-01" @default.
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- W2079968761 title "Implications of the ionizing continuum of 3C263" @default.
- W2079968761 doi "https://doi.org/10.1093/mnras/248.1.139" @default.
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