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Dynamics of relativistic radio jets in asymmetric environments [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 We have carried out relativistic three-dimensional simulations of high-power radio sources propagating into asymmetric cluster environments. We offset the environment by 0 or 1 core radii (equal to 144 kpc), and incline the jets by 0, 15, or 45 degree ...
Patrick M Yates-Jones +2 more
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A Galactic survey of radio jets from massive protostars
Monthly Notices of the Royal Astronomical Society, 2021 In conjunction with a previous southern-hemisphere work, we present the largest radio survey of jets from massive protostars to date with high-resolution (∼0.04 arcsec) Jansky Very Large Array observations towards two subsamples of massive star-forming ...
S J D Purser, M G Hoare, S Kurtz
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Annual Review of Astronomy and Astrophysics, 1984
On a examine les proprietes systematiques des jets radio et on s'interroge sur leur contribution a la comprehension des processus de transfert d'energie dans les sources extragalactiques.
Alan H. Bridle, Richard A. Perley
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On a examine les proprietes systematiques des jets radio et on s'interroge sur leur contribution a la comprehension des processus de transfert d'energie dans les sources extragalactiques.
Alan H. Bridle, Richard A. Perley
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Jets in Extragalactic Radio Sources
Science, 1984Observations now require that there be a continuous supply of energy to the giant extragalactic radio sources. These observations also suggest that this energy input may be in the form of streams or jets of gas emanating from the centers of galaxies and quasi-stellar objects. Current data indicate that the large-scale jet structures are not moving with
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Nature, 1981
Most radio sources are two-sided, but a minority appear onesided, 3C273 being the first-known and brightest example. There is no agreement1–4 on whether such sources are intrinsically one-sided, or are normal double sources, one half of which is hidden by Doppler effects.
R. G. Conway +3 more
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Most radio sources are two-sided, but a minority appear onesided, 3C273 being the first-known and brightest example. There is no agreement1–4 on whether such sources are intrinsically one-sided, or are normal double sources, one half of which is hidden by Doppler effects.
R. G. Conway +3 more
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Nature, 1979
The peculiar emission line object SS433 (refs 1–3) has variable radio emission and an angular size of
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The peculiar emission line object SS433 (refs 1–3) has variable radio emission and an angular size of
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The structure of the radio jets in 3C449
Nature, 1979High resolution observations of 3C449 show the presence of two highly collimated symmetric jets on each side of an unresolved core. The jets show considerable fine structure and polarisation. Measurements of the depolarisation suggest internal densities of ∼0.02 cm−3 and flow velocities of ≳1,000 km s−1.
R. A. Perley, A. G. Willis, J. S. Scott
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