Anisotropic Distribution of Space Pulsar Velocities
American Journal of Astronomy and Astrophysics
Volume 2, Issue 6-1, December 2014, Pages: 29-31
Received: Sep. 22, 2014; Accepted: Sep. 25, 2014; Published: Oct. 29, 2014
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Author
Igor Fedorovich Malov, P. N. Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Russia
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Abstract
On the base of new data it is shown that the observed proper motions and directions of the tangential velocities of pulsars manifest the extremely anisotropic distributions. These anisotropies cannot be explained by the structure of our Galaxy or by various types of solar motions. They can be caused by the cosmological vector potential and the action of the new force. This force must be stronger in higher magnetic fields. The positive correlation between tangential velocities Vt and surface magnetic fields of pulsars Bs is seen indeed. It is shown that the new force can provide pulsar velocities up to several thousands of km/sec.
Keywords
Pulsars, Proper Motions, Magnetic Fields, New Force
To cite this article
Igor Fedorovich Malov, Anisotropic Distribution of Space Pulsar Velocities, American Journal of Astronomy and Astrophysics. Special Issue:Global Anisotropy, Theory of Byuon, New Force, New Power System, Propulsion, Space Flights. Vol. 2, No. 6-1, 2014, pp. 29-31. doi: 10.11648/j.ajaa.s.2014020601.14
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