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On the Nature of the Geminga Pulsar

Published online by Cambridge University Press:  12 April 2016

D. Khechinashvili ,
G. Melikidze  and
J. Gil
D. Khechinashvili
Affiliation:
J. Kepler Astronomical Center, Pedagogical University, Lubuska 2, 65-265, Zielona Góra, Poland Abastumani Astrophysical Observatory, Al.Kazbegi ave. 2a, Tbilisi, 380060, Georgia
G. Melikidze
Affiliation:
J. Kepler Astronomical Center, Pedagogical University, Lubuska 2, 65-265, Zielona Góra, Poland Abastumani Astrophysical Observatory, Al.Kazbegi ave. 2a, Tbilisi, 380060, Georgia
J. Gil
Affiliation:
J. Kepler Astronomical Center, Pedagogical University, Lubuska 2, 65-265, Zielona Góra, Poland

Abstract

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The model provided that Geminga is an almost aligned pulsar, which is supported by the low-frequency observations. The model explains successfully most of the peculiarities of Geminga radio emission. In the frame of the same geometry we propose a mechanism for the recently detected optical pulsation from that pulsar.

Type
Part 6. Emission and Plasma Theory
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 423 - 424
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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