Results 301 to 310 of about 92,360 (324)
Ohm's Law, the Reconnection Rate, and Energy Conversion in Collisionless Magnetic Reconnection. [PDF]
Liu YH+14 more
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Correlations and Kappa Distributions: Numerical Experiment and Physical Understanding. [PDF]
McComas DJ, Livadiotis G, Sarlis NV.
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Macromolecular crystallography and biology at the Linac Coherent Light Source. [PDF]
Mous S+4 more
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The multiwavelength behaviour of BL Lacertae explained by a wiggling filamentary jet
Raiteri C.
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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
openaire +2 more sources
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
openaire +2 more sources
Astrophysics and Space Science, 2001
LS 5039 is a high mass X-ray binary whose optical counterpart is a bright (V = 11) star of 07 V((f)) spectral type, at an estimated distance of 3.1 kpc. The radio emission from LS 5039 is persistent and its radio spectrum is clearly non-thermal. Here we report VLBA and VLA observations which reveal that LS 5039 is resolved into bipolar radio jets ...
Marc Ribó+3 more
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LS 5039 is a high mass X-ray binary whose optical counterpart is a bright (V = 11) star of 07 V((f)) spectral type, at an estimated distance of 3.1 kpc. The radio emission from LS 5039 is persistent and its radio spectrum is clearly non-thermal. Here we report VLBA and VLA observations which reveal that LS 5039 is resolved into bipolar radio jets ...
Marc Ribó+3 more
openaire +2 more sources