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Sharper upper limits have been obtained in experiments designed to detect effects caused by the galactic vector potential.
These sharp limits from the non-observation of the effects caused by the galactic vector potential have been shown to be model dependent.
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The galactic vector potential can also be probed directly by measuring the torque exerted on a magnetized ring.
Although the galactic vector potential is very large because the galactic magnetic field exists on very long length scales, only the magnetic field is observable if the photon is massless.
It is likely that the polarization arises because the dust grains are partially aligned by the galactic magnetic field.
This cannot be realized by the galactic anisotropy.
But as G2 passed by this summer, the galactic center was conspicuously quiet.
The Grox will hate you for destroying their colonies, but apparently you get a +15 by breaking the galactic code.
Such a procedure enables the avoidance of contamination by sources from the Galactic plane and Galactic cirrus emission.
Reacceleration of cosmic rays produced by galactic sources on the galactic wind termination shock is considered.
Only those sources in the sky area surveyed by MSX, mostly in the Galactic plane, are left.
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