Hostname: page-component-7bb8b95d7b-w7rtg Total loading time: 0 Render date: 2024-10-01T09:54:49.391Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Gil, J.A., Khechinashvili, D.G., & Melikidze, G.I. 1998, MNRAS, 298, 1207 CrossRefGoogle Scholar
Lyubarskii, Y.E., & Petrova, S.A. 1998, A&A, 337, 433 Google Scholar
Malofeev, V.M., & Malov, O.I. 1997, Nature, 389, 697 CrossRefGoogle Scholar
Malov, I.F. 1998, Astron. Reports, 42, 246 Google Scholar
Vats, H.O., et al. 1999, MNRAS, 302, L65 CrossRefGoogle Scholar